The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless light distribution. The galaxy exhibits a concentrated central bulge, with a gradual decrease in luminosity outwards, displaying an approximately elliptical shape, with an aspect ratio that suggests it is closer to round than a cigar shape. There are no obvious spiral arms or disk-like structures visible. No signs of major mergers or significant tidal disturbances are observed; it looks like it may have experienced minor disturbance. The color is generally yellow-ish. This color suggests that the galaxy is primarily composed of older stars. The relatively high degree of smoothness is consistent with a galaxy where star formation has largely ceased and where the stellar population is dominated by older stars. 
