The galaxy presents as a relatively small, well-defined structure with a bright, concentrated central bulge. The overall shape appears elliptical, but with some subtle irregularities that suggest a disk component viewed at a high inclination. The bulge exhibits a smooth, featureless appearance. Faint spiral arms, or some form of extended disk-like structure, is hinted at but not clearly resolved. There are some irregularities in the symmetry of the faint outer regions that suggest potential tidal interactions or a minor merger event. There are no obviously visible dust lanes obscuring the core or disk. The color gradient indicates a relatively older stellar population, with a slightly bluer hue associated with the outer regions of the galaxy, suggesting some recent but low levels of star formation. There is a potential presence of a faint active galactic nucleus (AGN).
