The galaxy appears as a roughly circular, diffuse object. The light is concentrated towards the center, exhibiting a smooth, centrally-peaked light profile. The core region displays a bright yellowish-white hue, possibly indicating a significant population of older stars. Proceeding outward, the color shifts towards a redder tint. The light distribution suggests a primarily spheroidal structure, possibly an elliptical galaxy or a bulge-dominated spiral. However, there is no clear evidence of spiral arm structures or a prominent disk component in this image, possibly due to distance. Indications of minor disturbances are present, but they are not a large scale disruptive presence. The galaxy appears relatively isolated, without obvious signs of tidal interactions or ongoing mergers.
