The object is a spiral galaxy, viewed nearly edge-on from our line of sight. A prominent central bulge dominates its structure, exhibiting a smooth, concentrated luminosity profile that suggests an older stellar population. The bulge is elliptical and yellowish in color, indicative of relatively low star formation activity.

Surrounding the bulge, a fainter, more diffuse disk is observed. The disk appears flattened and elongated, which supports the edge-on perspective. The color of the disk grades towards a bluer hue compared to the bulge, hinting at the presence of younger, hotter stars and regions of ongoing star formation. There is no visible dust lane, suggesting that we are looking at a later type spiral galaxy.

There is no obvious evidence of any tidal interactions or merging events. The spiral arms are not clearly resolved, probably due to its edge-on orientation. No evidence of distinct star-forming regions can be seen. The galaxy appears to be a relatively undisturbed system.
