The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a notable color gradient, transitioning from a redder core region to a bluer outer halo. The central region appears slightly elongated, trending towards an elliptical shape rather than a perfect circular profile. No distinct spiral arm structures or prominent dust lanes are visible in the image. The galaxy appears relatively isolated, without obvious signs of major tidal disturbances or ongoing mergers, though a minor asymmetry or possible faint extension is observed on one side. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy, potentially an elliptical or lenticular system. The redder core and bluer outer regions suggest a possible radial variation in stellar populations, with older, redder stars concentrated centrally and younger, bluer stars more prevalent in the outer regions.
