The galaxy appears as an elliptical type, exhibiting a smooth, diffuse light distribution. The light is primarily concentrated in the central region, with a gradual decrease in intensity towards the outer edges, suggesting an older stellar population dominates its composition. The galaxy's shape is not perfectly circular but shows a slight elongation, tending toward a more flattened profile. There is no discernible spiral structure or dust lanes visible in this image. There appears to be a companion galaxy in close proximity to it. The light is yellow indicating an older, less active galaxy. It appears relatively undisturbed, without any major signs of tidal interactions or mergers, though minor disturbances cannot be ruled out. Its color is fairly uniform across its extent, suggesting a relatively homogeneous stellar population and a lack of ongoing significant star formation.
