The galaxy presents an elliptical morphology, appearing moderately elongated. It exhibits a smooth light distribution, with a noticeable concentration towards the center. The color profile indicates a redder core region, possibly indicative of an older stellar population, transitioning to a slightly bluer outer halo, which might suggest ongoing or recent star formation activity. There is no clear evidence of spiral arms or major disturbances, and the overall structure suggests a relatively evolved and quiescent system.
