The galaxy presents a primarily smooth morphology. It appears elliptical in shape, displaying a concentrated central bulge. The light profile suggests a gradual decline in luminosity from the center outwards. There is no apparent spiral structure or significant dust lane obscuration. The galaxy exhibits a reddish-yellow hue, indicative of an older stellar population. The overall appearance suggests minimal current star formation activity. There are no obvious signs of tidal disturbances or recent merger events.
