The galaxy presents as a somewhat elongated, elliptical morphology. A smooth and centralized bulge dominates the overall structure. The galaxy exhibits a yellowish-orange hue across its body, potentially indicating a population of older stars. There is little to no evidence of spiral arms or significant dust lanes, suggesting a lack of ongoing, large-scale star formation. Subtle irregularities in the outer regions might indicate minor gravitational interactions or recent accretion events, although the galaxy is generally undisturbed. Overall, it appears to be a relatively evolved system.
