The galaxy presents as a single, relatively smooth object. The central region exhibits a concentrated, bright core, suggesting a high density of stars. The overall shape appears somewhat elliptical, though deviations are present. The light profile gradually decreases from the center outwards, with no distinct spiral arms or bar structures visible. The color is predominantly yellowish-orange, indicating a population of older stars, although subtle color variations exist within the extended halo. Faint, diffuse features are possibly present in the outer regions, but these may be due to image artifacts or extremely faint tidal interactions. There is no apparent major ongoing merger activity, nor evidence of a prominent disk structure or significant dust lanes. Overall, this galaxy seems consistent with an early-type galaxy such as an elliptical.
