This galaxy exhibits a predominantly smooth morphology, with a slight elongation. The central region displays a bright, concentrated core that appears somewhat reddish in color, which could indicate a population of older stars or significant dust obscuration. Surrounding the core is a more diffuse, greenish halo. The color variation from red at the core to greenish in the outer regions may suggest differing stellar populations or varying levels of star formation activity. The lack of obvious spiral arms or a well-defined disk structure supports its classification as a possibly elliptical galaxy. There are no immediately apparent signs of major mergers or significant tidal disturbances, although a subtle asymmetry might hint at minor gravitational interactions in its past. The overall appearance suggests a fairly evolved system, but further spectroscopic analysis would be needed to fully characterize its composition and evolutionary state.
