The galaxy presents as a relatively smooth, elliptical object, with a concentrated central bulge. The core exhibits a bright, yellowish hue, suggesting a population of older stars. There is a gradual decrease in luminosity moving outward from the core, with the outer regions appearing more reddish, indicating the presence of potentially cooler, older stellar populations or dust obscuration. No distinct spiral arm structures or significant dust lanes are visible. The galaxy appears largely undisturbed, exhibiting no major signs of ongoing mergers or tidal interactions with other galaxies. The overall morphology suggests a mature galaxy that is not actively forming a large number of new stars.
