The galaxy presents as a somewhat compact object with a distinct, flattened, elliptical morphology. The light distribution is concentrated towards the center, suggesting a higher density of stars and/or a more massive central component. There is a bright central region which could indicate an active galactic nucleus or intense star formation. Some slight color variation is visible, with hints of bluer regions interspersed with redder components, potentially indicative of varying stellar populations or dust content across the galaxy. The overall smooth appearance of the galaxy suggests it is most likely an elliptical galaxy, with limited evidence of spiral arms or other features associated with disk galaxies. There may be some minor disturbances present.
