This galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a bright core that gradually fades into a more diffuse halo. The overall shape is generally elliptical, with a slight deviation from perfect circularity. There is little evidence of distinct spiral arms or a prominent disk structure. The color profile suggests an older stellar population, with a yellowish-white hue dominating the central region, transitioning to a slightly bluer tint in the outer edges of the halo. There are no clear signs of ongoing major mergers or significant tidal disturbances in this image, although subtle irregularities in the light distribution may indicate minor interactions or internal dynamics. The galaxy is estimated to be of intermediate mass. Its rate of star formation is estimated to be low.
