The galaxy appears as a concentrated, elliptical-like structure, displaying a smooth morphology with little evidence of spiral arms or significant disk features. The central region exhibits a bright, yellowish hue, suggesting a high concentration of older stars. The light gradually fades toward the outer regions, with the overall color becoming slightly redder. This may indicate a larger population of older stars at its periphery. The structure seems largely undisturbed, with no obvious signs of tidal tails or ongoing major mergers. It is moderately compact, exhibiting a rather round shape and no significant distortions or prominent features typically associated with active star formation.
