The galaxy presents as an elliptical morphology with a dominant, smooth spheroid component. The core exhibits a concentrated luminosity profile, appearing bright and yellowish-white, indicative of a population of older stars. A fainter, bluer haze surrounds the core, suggesting the presence of a younger stellar population, or possibly dust scattering blue light. The ellipticity of the galaxy is moderate, with a slight elongation along a preferential axis. There are no readily discernible spiral arms or prominent dust lanes, consistent with a relatively evolved system. Faint, extended emission is observed, indicating a diffuse halo surrounding the main body of the galaxy. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in the image.
