The galaxy presents as a single, centrally concentrated object with a smooth light profile. It appears highly symmetrical, exhibiting a nearly circular morphology, which could suggest it is an elliptical galaxy or a face-on spiral galaxy with a prominent bulge. The central region is significantly brighter than the surrounding areas, indicative of a high stellar density, possibly housing a supermassive black hole. There is a color gradient, with the core exhibiting a yellowish hue transitioning to a redder color in the outer regions. No distinct spiral arms, bars, or dust lanes are discernible. The overall structure suggests a galaxy that has undergone significant merging or is in a relatively quiescent state of star formation. No signs of tidal tails or ongoing interactions with other galaxies are observed, indicating the system is relatively isolated or has completed its merging process. The colors and morphology are consistent with a population of older stars.
