The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution appears elliptical in shape, with a high degree of symmetry. There is a lack of any discernible spiral arm structure or prominent dust lanes. The galaxy exhibits a color gradient, with a yellowish core gradually fading to a redder hue in the outer regions. This suggests a population of older stars dominates the central region, while the outer areas may contain a mix of stellar populations. No signs of any major mergers are visible in the galaxy.
