The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears primarily elliptical, showing little to no discernible disk structure. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population dominating the central region. Moving outward from the core, the color gradually shifts toward a redder tone. The galaxy's shape is largely spheroidal, and shows a slight deviation towards an in-between roundness. There are no apparent signs of a recent major merger event, though subtle irregularities in the outer regions suggest possible minor gravitational interactions. Star formation is present, but relatively low.
