The galaxy presents as a smooth, centrally concentrated structure with a slightly elongated, cigar-like shape. There is a distinct lack of spiral arm structure or prominent dust lanes visible. The central region appears brighter and more condensed, indicating a possible bulge component. Color gradients suggest that the core is old while the outer regions contain some younger stars. No signs of any major mergers, tidal tails, or strong disturbances are apparent in the morphology.
