The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears generally elliptical, with a noticeable lack of defined spiral arms or a prominent disk structure. The central region exhibits a bright, somewhat indistinct core, possibly indicating a high stellar density or active galactic nucleus. The light profile transitions smoothly from the core outwards. The galaxy displays a yellowish-white hue in its central regions, grading to a reddish tinge in the surrounding areas of the halo. This may indicate an older stellar population. There are potentially minor disturbances in the outer halo of the galaxy, though these are not overtly indicative of an ongoing major merger event. Overall, the galaxy seems to be a mature system, likely dominated by evolved stars, with a high degree of symmetry and structural regularity.
