This galaxy presents as a relatively small, disk-shaped system observed nearly edge-on. A prominent central bulge appears bright white, possibly indicative of a dense concentration of older stars. The disk itself exhibits a blue hue suggesting the presence of ongoing star formation, although it appears relatively smooth. There is a small amount of asymmetry visible, with some areas on the disk appearing slightly perturbed. Overall, the galaxy does not seem to be undergoing a major merging event. This system displays an overall smooth morphology, and lacks any major disturbances. 
