The galaxy presents as a generally smooth, elliptical morphology. Its light profile appears centrally concentrated with a gradual decrease in intensity towards the outer regions. The core region exhibits a yellowish-orange hue, suggesting a population of older stars. There is minimal evidence of spiral arms or significant dust lanes. Overall, the galaxy appears relatively undisturbed, lacking prominent tidal features or indications of a recent major merger event. There might be minor distortions or faint plume-like structures visible, but these features do not heavily impact the classification of the galaxy.
