The galaxy presents as a single, relatively homogenous object. Its overall morphology appears elliptical, showing a smooth light distribution without discernible spiral arms or a distinct disk. The central region displays a high concentration of light, which gradually fades towards the outer edges. There is a slight elongation. The color is generally yellow, indicating a population of older stars. No evidence of active star formation regions, such as blue knots or HII regions, is apparent in the image. The galaxy doesn't show any signs of being involved in a major merger or tidal disturbances.
