The galaxy presents an elliptical morphology, exhibiting a smooth light distribution. Its shape deviates slightly from perfectly circular, being somewhat elongated. The color indices suggest it is likely composed of an older stellar population, with lower levels of ongoing star formation. The galaxy shows no clear evidence of spiral arms or a distinct disk structure, fitting more into a classification as an elliptical galaxy. There is a possible merging event occurring, where there is an interaction of two bodies, causing a disturbance to each of the galaxy's structure. The outer regions are noticeably fainter, indicating a gradual decrease in stellar density away from the central bulge.
