The galaxy presents as a somewhat diffuse, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars. The surrounding region displays a gradual decrease in brightness, fading into the background. The morphology appears to be more smooth than spiral. There is a slight suggestion of possible minor tidal disturbances or interactions on one edge, but nothing is obviously merging with the primary structure. The color profile indicates a predominantly older stellar population as indicated by the yellow and reddish light, but some pockets of bluish light may indicate younger star formation. 
