The galaxy presents as a somewhat compact, roughly elliptical object. It exhibits a bright central core that is surrounded by a fainter, more diffuse halo or disk. Within the core, there is a very bright unresolved region. The outer regions are less defined, presenting as irregular in shape with a clumpy appearance. There appear to be faint extensions or tidal features suggesting possible past or ongoing interactions or mergers. The color gradients suggest that the central area is relatively bluer than the outer regions, indicating younger stellar populations in the center and older populations in the outskirts. Overall, the galaxy exhibits characteristics of a disturbed or actively evolving system.
