The galaxy presents as a relatively smooth, elliptical morphology with a central bulge that dominates the overall structure. The light distribution appears concentrated, with a gradual decrease in intensity moving outwards from the core. The shape of the galaxy is elongated, but not excessively so, appearing somewhere between round and cigar-shaped. There is a subtle hint of disk structure, but overall the galaxy appears to be dominated by a spheroidal component. There is no strong evidence of ongoing major mergers or significant tidal disturbances. A minor disturbance is possible. The color is somewhat red, suggestive of an older stellar population.
