The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity moving outward from the core. The color profile suggests an older stellar population, with a yellow-red hue dominating the galaxy's overall color. There appears to be little evidence of significant dust lanes or prominent spiral arm structures. The overall shape indicates the galaxy is more elliptical than disk-shaped. There's no apparent major merging or significant tidal disturbance present. The morphology suggests a galaxy that is fairly evolved, with a relatively low current star formation rate.
