This galaxy appears to be an elliptical galaxy. Its overall morphology is smooth and round, lacking any distinct spiral arms or a defined disk structure. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is a slight colour gradient, with the central region exhibiting a bluer hue in comparison to the outskirts, which present a more yellow colour. This could indicate a population of younger, hotter stars in the core, with older stellar populations dominating the galaxy's halo. There is no visible evidence of ongoing major mergers or significant tidal disturbances. The galaxy appears relatively undisturbed.
