The galaxy exhibits a relatively smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual decline in surface brightness outwards. The core region presents a yellowish-red hue, suggesting an older stellar population dominated by red giant stars. The outer regions show a shift toward greener colors, potentially indicating the presence of some younger, hotter stars, albeit at a low star formation rate. There is no clear evidence of spiral arm structure or significant dust lanes, although a slight asymmetry is visible. No signs of a major merger event are present, although there may be some minor disturbances in the halo. The overall shape is approximately round, with a diameter that suggests it is a medium sized galaxy.
