The galaxy presents as a centrally concentrated object, exhibiting a smooth, relatively featureless morphology. The light distribution appears close to symmetrical. Its color is distinctly yellowish-orange, indicating a stellar population dominated by older, redder stars. The galaxy's overall structure does not suggest any ongoing major mergers or significant tidal disturbances, although there may be a subtle asymmetry on one side suggesting a minor interaction. The overall shape is elliptical, and the light falloff appears gradual, consistent with a diffuse halo component.
