The galaxy presents as a somewhat elongated, cigar-shaped structure with a relatively smooth, diffuse appearance. There is a distinct color gradient; the central region exhibits a bluer hue, suggesting the presence of younger stellar populations and possibly ongoing star formation, while the outer regions appear redder, indicative of older stars. The lack of defined spiral arms or a prominent central bulge points towards the galaxy being an elliptical or lenticular type. There are no signs of major disturbances or significant tidal features, suggesting the galaxy is relatively isolated or has completed any recent mergers.
