The galaxy presents as a centrally concentrated system with a relatively smooth morphology. The light profile appears to be dominated by a spheroidal component, showing a high degree of central bulge dominance. The galaxy exhibits a nearly circular appearance and is categorized as being well-rounded. A faint, diffuse halo extends outwards from the central region, and the color profile indicates the presence of a stellar population showing a slightly evolved system. No prominent spiral arm structures are apparent, and the galaxy does not obviously show any signs of major ongoing mergers or strong tidal disturbances. Faint signs of minor asymmetry could suggest tidal interactions or minor disturbances.
