The galaxy presents as a centrally concentrated object with a largely smooth morphology. There is an observed radial gradient in color, with the core region exhibiting a bluer hue compared to the more reddish extended outskirts. The light distribution appears approximately round, showing no strong evidence for a prominent disk or spiral arm structure. Faint extensions are present, potentially suggesting minor tidal disturbances or interactions with other objects, though a merger scenario cannot be conclusively confirmed from this image alone. Given the overall smoothness and central concentration, the galaxy could be classified as an early-type system. There is a possibility the galaxy is forming new stars but the rate is low.