The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated central bulge. It exhibits a generally round morphology, with a slight deviation towards an in-between shape, showing a smooth distribution of light. The galaxy appears to have no distinct features, such as spiral arms or strong tidal disturbances. It is characterized by an overall yellowish-white hue, which is indicative of an older stellar population, with little evidence of ongoing major star formation. The light concentration suggests that the galaxy is composed of a stellar population that is mostly old. There is no apparent disk-like structure to the galaxy.
