The galaxy presents as a fairly smooth, centrally concentrated object. The light is distributed relatively evenly throughout the galaxy, with a strong concentration at the core. The overall shape is elliptical in projection, with a high degree of roundness. There is no evidence of spiral arms or a prominent disk structure. The galaxy exhibits a color gradient, transitioning from a slightly bluer hue in the outer regions to a yellower, potentially redder color towards the core. This color gradient may indicate a difference in stellar populations or dust content between these regions. There are no obvious signs of recent or ongoing major mergers or tidal disturbances.
