The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The core exhibits a pronounced red color, indicative of an older stellar population. Surrounding the core, there's a less defined, more diffuse halo showing a subtle gradient toward bluer wavelengths. This suggests the presence of a younger stellar population in the outer regions, although not prominent. There is a slight indication of minor disturbances. The galaxy appears relatively isolated, with no obvious signs of recent or ongoing major mergers.
