The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology with a high degree of central concentration. The light profile shows a gradual decline in brightness from the core outwards. The color gradient suggests a centrally located population of older stars, indicated by the yellowish-white hue in the core, transitioning to a bluer color in the outer regions. This suggests some ongoing star formation, albeit at a low rate, in the galaxy's outskirts. There is no visible evidence of spiral arms or a defined disk structure. No significant signs of tidal disturbances or ongoing mergers are apparent in the image, indicating the galaxy is relatively undisturbed. The galaxy possesses a relatively small size.
