The galaxy presents as a centrally concentrated object with a smooth overall appearance. The light distribution indicates a generally elliptical morphology, although there is a slight asymmetry, possibly suggesting the presence of a weak disk component or a minor tidal interaction. The core region exhibits a bright, relatively compact concentration of light. The outer regions fade gradually into the background, lacking any distinct, defined edges. There are no clearly discernible spiral arms or prominent dust lanes. The color profile is mostly uniform across the galaxy, with a subtle shift towards bluer hues in the outer regions, possibly indicating a slightly younger stellar population in these areas. There is no evidence of a strong ongoing merger, but some subtle distortions might suggest a minor disturbance or recent interaction.
