The galaxy presents as a generally smooth, somewhat rounded structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards its outer regions. There is a hint of a possible disk-like feature, but it is not clearly defined. The galaxy's color profile suggests a population of older stars, with a redder hue dominating the overall appearance. There are slight color variations across the galaxy, possibly indicating regions with differing stellar populations or dust content. There may be signs of a minor disturbance in the morphological structure, potentially indicative of a past or ongoing interaction with a smaller companion galaxy. Overall, the galaxy appears to be relatively isolated and shows no signs of a recent major merger event.
