The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central region with a gradual decrease in luminosity towards its outer edges. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears somewhat rounded in shape, with no obvious signs of major disturbances or mergers. Its color profile suggests a evolved stellar population. There are no apparent star-forming regions. The galaxy has some level of star formation but low specific star formation rate.
