The galaxy presents as a single, concentrated object. Its morphology appears largely smooth and elliptical, lacking prominent spiral arms or a distinct disk structure. The light distribution suggests a centrally concentrated luminosity profile, with intensity decreasing gradually toward the outer regions. There is a slight elongation in shape, but overall, it appears rather rounded.

The core of the galaxy exhibits a yellowish hue, indicative of a population of older stars. The outer regions display a slightly bluer color, which may suggest the presence of a younger stellar population. The overall color suggests a population that is dominated by older stars with a small amount of ongoing star formation. I do not observe any signs of major mergers or significant tidal disturbances.
