The galaxy appears to be a relatively smooth, elliptical or lenticular type. Its morphology presents a centralized, concentrated light profile, indicating a large bulge component. The shape is approximately round, with a slight elongation. There's no evidence of spiral arms or a pronounced disk structure. The color gradient suggests a population of older stars, with a redder hue dominating the outer regions and a more yellow-white color in the core, indicating potentially different stellar populations or metallicities across the galaxy. There's no obvious sign of recent or ongoing major merging events, though subtle irregularities may suggest a minor interaction in the past. Star formation rate appears low. Overall, the galaxy presents a quiescent, evolved system.
