This galaxy exhibits a smooth, slightly elliptical morphology. A central bulge is discernible, showing a concentrated region of light. The outer regions appear more diffuse, and the galaxy lacks any prominent spiral arm structures. Color gradients suggest a redder population in the core transitioning to bluer components in the outskirts. No obvious signs of a major ongoing merger are visible, however, there are subtle features that indicate a possible minor disturbance in its gravitational environment. The overall appearance is consistent with that of an early-type galaxy.
