The galaxy presents as a lenticular or early-type spiral galaxy. Its morphology suggests a primarily smooth structure with minimal visible substructure. The galaxy is characterized by a cigar shape. There are no obvious signs of spiral arms or a prominent central bulge. The light is concentrated towards the center, fading gradually outwards. The galaxy appears relatively undisturbed, with no signs of ongoing major mergers or tidal disruptions. The color suggests a population of older stars, with a relatively low rate of star formation.
