The galaxy presents with a primarily elliptical morphology, showing a relatively smooth, albeit not entirely featureless, structure. The central bulge is bright and concentrated, with a distinct, diamond-like, high-intensity core region. A faint disk-like structure appears to surround the central bulge, though it is not sharply defined.

There appears to be a very slight disturbance or asymmetry in the outer regions of the disk, possibly indicating a minor interaction or past merger event. However, distinct tidal tails or other prominent merger features are not apparent in the image. The color profile suggests a varied stellar population, with a brighter, potentially younger component in the central regions.

The overall form suggests a galaxy undergoing a transition from a spiral structure to a more elliptical one, or a galaxy where ongoing interactions are subtly shaping its morphology.
