The galaxy presents as a centrally concentrated, elliptical morphology with a relatively smooth profile. Its core exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. The galaxy's shape is elongated, with a clear major and minor axis indicating a non-spherical structure. There is a slight color gradient from the center outwards, transitioning to a fainter, bluer hue in the outer regions. This may indicate the presence of a younger stellar population in the outskirts, although the effect is subtle. The overall structure appears undisturbed, with no obvious signs of recent major mergers or tidal interactions. The galaxy lacks distinct spiral arms or prominent dust lanes, which is consistent with its elliptical classification.