The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth overall appearance. There is a high degree of radial symmetry, indicating a lack of significant spiral arms or other pronounced disk features. The light profile appears relatively uniform, with a gradual decrease in brightness from the center outwards. There may be an extremely slight color gradient, with a slightly more yellow hue toward the core and a fading into more reddish tones further out, consistent with an older stellar population. No obvious signs of recent or ongoing major mergers are detected, though a slight asymmetry is present, potentially caused by a minor interaction. The galaxy's shape appears more spheroidal than highly elongated.
