The galaxy presents as an elliptical-like structure, exhibiting a centrally concentrated luminosity profile. The core region appears yellowish-red, potentially indicating an older stellar population. Moving outward from the center, the galaxy exhibits a subtle color gradient, transitioning towards a slightly bluer hue. This suggests the presence of a younger stellar population in the outer regions, perhaps from recent minor star formation. There is some suggestion of asymmetry in the outer regions. No prominent spiral arms are observed, and the overall morphology seems generally smooth, but is somewhat disturbed. The object's shape is between round and elongated.
