The galaxy presents a relatively compact morphology. The central region is dominated by a bright, concentrated core, suggesting a significant concentration of stars or potentially an active galactic nucleus, though no specific jetting is visible. The galaxy exhibits a somewhat elliptical shape, with a noticeable, though subtle, disk-like component extending outward from the central bulge. The overall color appears to be a relatively blue/white hue, indicating the presence of a population of young, hot stars, especially concentrated in the inner region. Possible minor disturbance to the upper right. A general indication of an interacting system may be reasonable. The outer regions appear fainter and fuzzier, which may represent the outer halo of the galaxy or tidal debris. There does not appear to be prominent spiral arm structure, suggesting either a smooth distribution of stars or that any arms may be too faint to resolve at this distance.
