The galaxy presents a generally smooth and centralized morphology. The central region appears bright and concentrated, displaying a yellowish hue, potentially indicative of an older stellar population. Fainter, bluish colors present in the outer regions may indicate star formation at the outer edges of the galaxy, or at least a younger population of stars at the outer edges. The overall shape appears somewhat elliptical but approaching a disk-like structure; it's more of a lens-like galaxy. No distinct spiral arms or strong bar features are immediately discernible. There are no strong disturbances or tidal tails observed which would indicate recent major merger activity. It would appear the galaxy has gone through no recent major mergers. Minor asymmetry or disturbance is subtle or absent.
