The galaxy presents an elliptical morphology, appearing somewhat elongated in shape. The light profile suggests a smooth distribution with a concentration towards the center, indicating a relatively old stellar population. There is no clear evidence of spiral arms or significant dust lanes. The central region displays a yellowish hue, possibly indicative of older, cooler stars. The outer regions show a slight transition to a bluer color, which could be a sign of younger stars, although they don't seem to be as active. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions. The galaxy doesn't seem to be extremely massive and has a relatively low star formation rate.
