The galaxy presents as a relatively smooth, centrally concentrated object, with a somewhat round shape. A slight elongation is discernible, but it does not appear significantly cigar-shaped. There is some suggestion of an interaction, though it is a minor disturbance. The light profile exhibits a gradual decline from the central core. The color is indicative of an older stellar population, being redder in comparison to typical spiral galaxies. There is evidence of moderate star formation.
