This galaxy presents a relatively compact, nearly circular morphology. Its core is bright, with a pronounced blue color, indicative of a region with potentially active star formation or a luminous active galactic nucleus. The outer regions of the galaxy appear less defined, with a diffuse halo-like structure surrounding the central bright core. There is a subtle color gradient observed, with the core presenting a bluer hue than the outer halo, which tends towards redder tones. This redder hue in the outer halo suggests an older stellar population. The overall structure lacks clear spiral arms or a prominent disk, which is also suggested by the round morphology. I note that there appears to be some interaction or tidal disturbances at play, seen by slight irregular shapes on the lower part of the galaxy.
