The galaxy appears to be a relatively bright, elliptical type, with a smooth, concentrated light profile. The central region exhibits a yellowish-red hue, possibly indicating an older stellar population or dust obscuration. Surrounding the core, there is a more diffuse, bluish halo, suggestive of younger stars or ongoing star formation at a lower rate. The galaxy is generally round in shape, showing no obvious signs of spiral arms or significant tidal disturbances. There may be a minor irregularity in the outer regions on one side, but no major mergers or interacting companions are visible. The overall color suggests a mix of stellar populations, with older stars dominating the core and younger stars sparsely distributed in the outer regions. The estimated size appears to be moderate, and the light output is moderately high.
