The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing nearly round but possibly tending towards a slightly elongated shape. There is no apparent evidence of spiral arm structure or significant disk-like features. The core exhibits a bright, concentrated region, potentially indicating an active galactic nucleus or a high density of stars. There appears to be a second area of high concentration within the object, indicating a possible recent disturbance in the galaxy. The color profile suggests a population of older stars, with a reddish hue dominating the outer regions and a slightly bluer, yet still relatively old, population towards the center. Overall, the galaxy appears to be a relatively massive, early-type system with minimal ongoing star formation. The absence of strong tidal features or significant morphological distortions suggests it is not currently undergoing a major merger event, although there appears to be a small disturbance in the core.
