The galaxy appears as a relatively smooth, elliptical object with a concentrated central bulge. The color gradient suggests a population of older stars, exhibiting a yellowish-red hue concentrated towards the core. The outer regions show a faint blue tinge, potentially indicating a small amount of younger stellar population. The morphology is generally round, lacking any visible spiral arms or bar structures. There are no indications of any major mergers or significant tidal disturbances. Overall, the galaxy presents as a mature, relatively undisturbed system.
