The galaxy presents a roughly elliptical morphology with a bright, concentrated core. The galaxy exhibits a smooth light distribution, suggestive of a relatively old stellar population. There is a slight color gradient visible, with the core appearing more yellow/orange and the outer regions having a hint of bluer hues. The overall structure indicates the galaxy is not actively undergoing a major merger. There might be a minor disturbance in the structure, but the galaxy is predominantly smooth and symmetrical.
