The galaxy presents a flattened, disk-like structure. The central bulge appears bright and concentrated, with a smooth texture indicative of an older stellar population. A faint disk is visible extending outward from the bulge, displaying a relatively low surface brightness. Hints of spiral arm structure may be present, but are not well-defined due to the galaxy's viewing angle. The galaxy exhibits a color gradient, with the bulge appearing more yellow/white, suggesting older stars, while the disk shows a slightly bluer tint, implying a younger stellar population and possible ongoing star formation. Overall, the galaxy appears to be an intermediate-mass system exhibiting characteristics of both spiral and lenticular galaxies. There is a slight indication of a minor disturbance, but it could be easily considered undisturbed, with no evidence of a recent major merger event. The galaxy is viewed nearly edge-on.
