The galaxy exhibits a generally smooth morphology, with a slight elongation, appearing somewhere between round and cigar-shaped. It presents a central bulge that appears bright and concentrated, and the surrounding disk appears smooth and relatively featureless. A slight blue tint suggests the possibility of ongoing star formation, although the galaxy appears predominantly redder in color, implying a population of older stars. There is no indication of any significant mergers or major disturbances, suggesting that the galaxy is relatively isolated and undisturbed.
