The galaxy presents as an elliptical morphology. The light is concentrated centrally, with a smooth, gradual decrease in surface brightness moving outwards. The core region exhibits a yellowish hue, suggesting an older stellar population. The outer regions appear slightly bluer, hinting at more recent or ongoing star formation, although the overall color profile indicates that star formation rates are low. There is no clear indication of a disk-like structure, spiral arms, or significant dust lanes. There is no strong evidence of any major merger events, tidal tails, or other disturbances. The shape tends to be round. It appears to be a relatively isolated system.
