The galaxy presents a largely smooth morphology with some disk-like features. The galaxy core shows a concentrated luminosity gradient, appearing bright and reddish, likely indicating an older stellar population or significant dust obscuration. The surrounding halo exhibits a bluer hue, possibly indicative of a younger stellar population or ongoing star formation, though it appears relatively quiescent. Overall, the galaxy displays a moderately elliptical shape. The image suggests a system that is not currently undergoing any major mergers. A minor disturbance is possible.
