The galaxy presents a moderately smooth, elliptical morphology. A significant portion of its light appears concentrated in a central, diffuse bulge exhibiting a yellowish hue, suggesting a population of older stars. Substantial tidal disruption is evident, with a second object in the process of merging with the central object. Broadly, the galaxy is relatively compact, measuring roughly 9 kiloparsecs across. Its low star formation rate, combined with the presence of an older stellar population, indicates that the galaxy is likely a relatively quiescent system.
