The galaxy presents as a primarily smooth, ellipsoidal structure, exhibiting a relatively concentrated central bulge. There is a faint disk surrounding the central region.

The color distribution indicates a yellow to red hue, suggesting an older stellar population and potentially low star formation activity. No significant dust lanes or spiral arm structures are readily apparent, further supporting the interpretation of a later-type system. There are no signs of tidal features or major disturbances that may indicate a recent merger event.
