The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated central bulge. There's a noticeable color gradient, transitioning from a brighter, possibly older stellar population in the core to a slightly bluer halo. Some faint, diffuse features are visible in the outer regions, potentially indicating minor disturbances or recent accretion events. The galaxy appears somewhat rounded, although not perfectly spherical. There is no prominent disk or spiral arm structure visible. The estimated mass of the galaxy is substantial, with signs of low-level star formation within.
