The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth and somewhat diffuse appearance. The core region exhibits a higher luminosity, suggesting a greater density of stars or a more active galactic nucleus. The overall shape is moderately elongated, appearing somewhere between round and cigar-shaped, without any obvious spiral arm features or significant disk structure. There is no strong evidence of recent or ongoing major mergers or tidal disturbances. The galaxy displays a gradual decrease in surface brightness from the center outwards, lacking significant substructure or distinct knots of star formation in the outer regions. The color profile indicates a bias towards redder wavelengths across the galaxy, which may indicate an older stellar population.
