The galaxy presents a roughly elliptical morphology, displaying a centrally concentrated luminosity profile. The core region exhibits a bright, relatively unresolved appearance, suggestive of a high stellar density and potential presence of an active galactic nucleus. Overall the galaxy appears smooth with a hint of a disk like structure. There are a few slight disturbances in the morphology suggesting a possible recent minor or major merger. The outer regions gradually fade into the background, showing a diffused halo component. There is a slight shift towards redder hues in the lower region of the galaxy suggesting dust lane or a possible tidal tail.
