The galaxy presents a roughly elliptical morphology, suggestive of a disk-dominated system. Its nucleus appears bright and concentrated, indicating a significant bulge component, though the surrounding disk is not negligible. Faint spiral arms are visible, though they are somewhat indistinct, possibly due to the viewing angle or a relatively smooth stellar distribution. The overall color suggests a mix of stellar populations, with a tendency toward bluer colors in the outer regions, which may indicate ongoing star formation. The galaxy does not display any obvious signs of major mergers or strong tidal disturbances. Its light profile suggests that it is a relatively normal spiral galaxy.
