The galaxy presents as a relatively smooth and rounded structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is a subtle color gradient, with the central region exhibiting a slightly yellower hue, suggesting a population of older stars. Fainter, bluer regions may be present in the outer areas, potentially indicative of younger stellar populations. No obvious spiral arms or distinct features such as bars or rings are discernible, suggesting a galaxy dominated by a spheroidal component. There may be minor disturbances in the overall light profile.
