The galaxy presents as a relatively smooth, centralized object. It exhibits a moderately elliptical morphology, appearing somewhat flattened but not highly elongated. The central region is brighter and more condensed, suggesting a prominent galactic nucleus or bulge. There is a subtle color gradient, with the central area exhibiting a yellowish hue transitioning to a bluer color towards the outer regions. This might indicate a difference in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars distributed in the outer regions where star formation is still happening. The outer edges are not sharply defined, fading gradually into the background sky. There is no clear evidence of spiral arms or a distinct disk structure. The overall appearance indicates that this galaxy is likely a massive system, and possibly in the later stages of its evolution. There may be hints of minor disturbances or faint tidal features surrounding the galaxy, but the image resolution limits definitive conclusions.
