The galaxy presents as a disk-shaped structure, elongated in appearance with a moderate degree of oblateness. Its morphology suggests an intermediate type between elliptical and spiral. The central bulge appears relatively smooth and featureless, exhibiting a concentrated distribution of light. The overall color profile is suggestive of an older stellar population, with a noticeable redder hue dominant throughout the galaxy's primary structure. There are indications of some disturbance to the shape of the galaxy, possibly from past interaction or some other merger event. Patches of bluer light are visible in the outer regions of the galaxy disk, hinting at regions of ongoing star formation.
