The galaxy presents a largely smooth, elliptical morphology. It appears as a concentrated spheroid of light with a noticeable yellow-orange hue, suggesting a population of older stars dominating its composition. There is a slight elongation, hinting at a shape somewhere between spherical and cigar-shaped. No distinct spiral arms or bars are visible. Slight irregularities are apparent along the edges, hinting at possible minor gravitational interactions or recent merger activity. Some possible dust lanes or slight color variations are also visible near the periphery.
