The galaxy appears as a somewhat diffuse, moderately bright object. It exhibits a flattened, disk-like structure, though it does not present a distinct spiral arm pattern. The central region appears slightly more concentrated and luminous, possibly indicating a bulge. A blue tint is observable across the galaxy, perhaps suggesting active star formation. There are no clear signs of strong tidal disturbances or major mergers in progress, though some mild asymmetry is present. It seems the galaxy is undergoing a period of relative quiescence, without significant ongoing interactions, although some mild disturbance cannot be ruled out. The overall morphology suggests a transition object, possibly between a disk and a more elliptical galaxy.
