This galaxy exhibits a generally elliptical morphology, though some distortion and features are apparent. The central region presents a bright, concentrated luminosity, suggestive of a significant stellar population or an active galactic nucleus. Moving outward from the core, the light appears to gradually diminish with an overall smooth distribution. Hints of a disk-like structure are visible, oriented close to edge-on. There is some subtle asymmetry on the outskirts, potentially indicating minor gravitational interactions or internal disturbances. A faint, greenish patch along one edge indicates possible localized star formation.
