The galaxy presents as a generally smooth object, with a concentrated central bulge. The color suggests an older stellar population. There is a hint of extended structure surrounding the main body, perhaps a diffuse halo or faint tidal features, but it's not well-defined. The galaxy appears to be generally elliptical in shape, exhibiting a high degree of rotational symmetry. There is no obvious indication of a strong disk component, though the outer regions show a slight flattening. No significant merging activity is apparent.
