The galaxy presents as a relatively faint, diffuse object. Its morphology appears to be disk-like, though the structure is somewhat disturbed or irregular. There is a noticeable blue hue throughout the galaxy, suggestive of ongoing star formation, particularly within the central region. It also shows hints of a possible ongoing or recent merger event, evident by an asymmetry in the overall shape and a possible tidal tail or disturbed structure extending from one side. The galaxy is moderately compact, implying a likely average mass.
