The galaxy presents a somewhat diffuse, elliptical appearance with a prominent central bulge. The overall color profile indicates a possible blend of stellar populations. The central region appears bright, indicative of a high concentration of stars or an active galactic nucleus. Faint, extended structures are observed surrounding the central bulge, potentially representing a disrupted or ongoing minor merger event. The galaxy exhibits a smooth luminosity distribution, yet with slight asymmetries suggesting possible tidal disturbances. There is no clear evidence of defined spiral arms or a distinct disk structure.
