The galaxy presents a generally elliptical morphology. A bright, concentrated core region dominates the central part of the galaxy. There is some evidence of a faint, diffuse halo extending beyond this core region, indicating a smooth transition in luminosity. The light distribution appears relatively uniform, with no prominent spiral arms or distinct structural features. There is a slight bluer coloring in the extended areas, but is it mostly yellow and red. Overall, the galaxy appears relatively evolved with ongoing star formation, indicative of an elliptical galaxy type. Based on the morphology, it would be classified as a relatively large early-type galaxy. There seems to be a possible merging event with a second smaller galaxy very close to the initial larger one, but further evidence may be necessary to confirm.
