The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish hue, which gradually fades into a diffuse halo. No distinct spiral arms or bar structures are discernible. The shape is slightly elongated, appearing more "in between" round and cigar-shaped. There is no obvious evidence of major mergers or significant tidal disturbances, although subtle irregularities in the outer halo cannot be ruled out at this resolution. The galaxy appears relatively isolated in this field of view. Color gradients suggest older stellar populations dominate, with potentially ongoing, yet subdued, star formation activity in the central regions.
