The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light profile. Its overall shape is largely spheroidal, with a high degree of circular symmetry. The core region is bright and appears yellowish or golden in color, indicating a population of older stars. There is a slight color gradient towards the outer regions, which appear marginally redder but this effect is minimal. No distinct dust lanes, spiral arms, or other features associated with actively star-forming galaxies are visible, consistent with a relatively quiescent system. The overall structure suggests a galaxy that has undergone significant merging activity in the past, resulting in its current smooth and rounded morphology. There is no strong evidence for ongoing interactions or tidal disturbances in the immediate vicinity.
