The galaxy presents as a distinct, elongated form, oriented approximately horizontally across the frame. It appears to be an edge-on disk galaxy. The primary axis of the galactic disk displays a gradation in luminosity and color. The central bulge region is the most luminous, with a noticeable concentration of light. This area exhibits a yellowish-white hue, suggestive of an older stellar population. Progressing outward from the bulge towards the edges of the disk, the luminosity gradually decreases. The outer regions of the disk show a slight bluer tint, potentially indicating the presence of younger, hotter stars.

The disk appears relatively smooth, with no obvious major spiral arm structures visible at this resolution. There is a subtle indication of dust lanes or obscuring material along the plane of the disk, although they are not sharply defined. There is no apparent tidal distortion or indications of a major ongoing merger event. However, there may be a subtle asymmetry in the outer regions of the disk, suggesting a possible minor interaction or disturbance in the past. The galaxy displays a well-defined, flattened structure characteristic of edge-on spiral or lenticular galaxies.
