The galaxy presents as a moderately inclined spiral, possibly nearing an edge-on orientation. It exhibits a distinct central bulge, characterized by a yellowish-white hue, which suggests an older stellar population. This bulge seems relatively smooth, indicating a lack of significant recent star formation in that region.

Extending outward from the central bulge, a faint, bluish disk is visible, which suggests the presence of younger, hotter stars and ongoing star formation. The disk appears relatively uniform in color, although there may be some subtle variations in surface brightness across its length. The overall structure appears somewhat undisturbed, without prominent signs of major mergers or tidal interactions. There might be a hint of slight asymmetry in the outer regions of the disk, suggesting a potential minor interaction or internal disturbance, but this could also be due to observational factors.
