The galaxy presents as an elongated, elliptical structure, exhibiting a smooth, relatively featureless appearance. The central region displays a concentrated luminosity, suggesting a prominent galactic bulge. The light distribution fades gradually from the core towards the outer edges. The overall color profile appears redder towards the center, possibly indicating a population of older stars, with bluer hues at the edges suggesting the presence of younger stars. There is an indication of minor tidal disruption, with a very slight plume structure on one side.

