The galaxy presents as a relatively smooth, centrally concentrated object. The core region is characterized by a bright, yellowish-white light emission, suggesting a dominant population of older stars. There is a subtle color gradient observable, with the outer regions exhibiting a slightly redder hue compared to the core. The overall morphology suggests a fairly round, elliptical shape, lacking any obvious spiral arm structures or significant disk features. There's no visual evidence of any major mergers or strong tidal disturbances affecting its structure, though there may be some minor asymmetries or irregularities in the outer halo that hint at a possible interaction history. The apparent lack of significant blue color suggests a relatively low star formation rate, although some residual star formation might still be present.
