The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall color is consistent with an older stellar population. The light appears to be concentrated towards the center, suggesting a higher density of stars in the core. There is a hint of asymmetry or minor disturbances in the outer regions, possibly indicating past or ongoing interactions. The galaxy does not appear to exhibit any prominent spiral arms or distinct features associated with active star formation, although some blue light is present. It shows characteristics of a fairly massive system.
