The galaxy presents as a relatively smooth, elongated structure. Its morphology appears to be that of a lenticular or early-type spiral galaxy, possibly seen nearly edge-on. There is a suggestion of a bulge component, though it is not distinctly prominent. The light distribution is concentrated towards the center, fading gradually outwards. There is little evidence of spiral arms or significant star formation regions based on the color. Its low redshift and absolute magnitude implies a moderate mass. There are hints of minor disturbances that could be indicative of a past merger or interaction, but these are subtle. The galaxy's light profile is more extended along its major axis, resulting in the observed cigar shape. The overall color suggests a population of older stars.
