The galaxy presents as a lenticular or possibly an elliptical galaxy, viewed nearly edge-on from our vantage point. It appears centrally condensed, exhibiting a bright nucleus with light gradually diminishing outwards, suggesting a relatively smooth light distribution. There is a hint of a disk-like structure, though obscured by its near edge-on orientation, and a notable lack of distinct spiral arms or irregular features. The galaxy displays a pale yellow-white hue, potentially indicative of an older stellar population with lower rates of active star formation. There appears to be a slight asymmetry in the outer regions, possibly due to tidal interactions or past mergers, but with no clear tidal tails present. The outer regions suggest a gradual fading of the light profile.