The galaxy presents as a somewhat elliptical structure with a noticeable central bulge, exhibiting a smooth light distribution. The orientation is such that we observe the galaxy at an angle, not quite edge-on but significantly tilted. The primary color is a yellowish-white, concentrated in the central region, suggesting an older stellar population. The outer regions of the galaxy show a subtle blue tint, indicating the presence of some younger, hotter stars. There is a lack of prominent spiral arm structure or distinct features, hinting at a later-type galaxy. The galaxy exhibits a relatively high Sersic index, which indicates a steep concentration of light. This is consistent with a galaxy whose structure is dominated by its bulge. There appear to be some minor disturbances in the outer disk of the galaxy.
