This galaxy exhibits a generally smooth morphology, appearing mostly featureless. The light distribution suggests an elliptical shape with a moderate degree of elongation. The central region displays a slightly brighter, redder core, transitioning to a bluer hue in the outer regions. There is no apparent spiral structure or significant disk component visible. The galaxy appears relatively isolated, showing no signs of major tidal interactions or ongoing mergers. Minor disturbances might be present, though not overtly noticeable. The overall color gradient implies a difference in stellar populations, with older, redder stars concentrated toward the center and younger, bluer stars in the outskirts. Overall, a lenticular or elliptical classification is likely.
