The galaxy appears as a moderately bright, disk-shaped structure with a well-defined central bulge. There is a noticeable color gradient, with the central region exhibiting a yellowish-white hue, suggestive of an older stellar population. A ring-like structure surrounds the bulge, appearing more blueish in color. This is consistent with younger stars and ongoing star formation. Evidence of disturbances is present in the form of a slightly irregular disk shape and subtle asymmetries in the light distribution. There are several faint tidal tails present. The galaxy does not present a highly disturbed morphology, therefore it is likely undergoing a minor interaction or recent minor merger.
