The galaxy presents as a centrally concentrated, relatively smooth object. It appears elliptical in shape, exhibiting a high degree of roundness. There is a noticeable color gradient, with the core region displaying a yellowish-white hue, suggesting a population of older stars. Progressing outwards, the color shifts to a slightly bluer tint in the surrounding regions. The absence of distinct spiral arms or a prominent disk indicates a low degree of structural complexity. The overall morphology suggests a relatively evolved system, potentially classified as an early-type galaxy, devoid of major ongoing star formation. No significant signs of tidal disturbances or interactions with other galaxies are apparent in the immediate vicinity. The galaxy's light profile appears to decrease smoothly from the center to the outer edges, consistent with a spheroidal distribution of stars.
