The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse profile. The core region exhibits a high surface brightness, indicating a dense stellar population. Moving outwards from the core, the luminosity gradually decreases, and the outer regions appear fainter and more diffuse. There appears to be a slight elongation, resulting in a shape somewhere between perfectly circular and cigar-shaped. The color profile suggests an older stellar population, with a yellowish-red hue dominating the overall appearance, which is consistent with minimal ongoing star formation.
