The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, with a noticeable decrease in luminosity towards its outer regions. The color profile suggests a population of older stars, with a dominant yellowish-orange hue in the core region, possibly indicating a higher concentration of evolved stars. There is a subtle greenish tint in the surrounding regions, potentially indicating some ongoing, albeit weak, star formation activity or a contribution from ionized gas. No clear spiral arm structures or dust lanes are discernible. The overall morphology suggests a galaxy that is not currently undergoing major mergers or significant interactions.
