The galaxy presents a largely smooth, elliptical morphology. There is a slight elongation, though it is generally rounded in appearance. The central region exhibits a concentrated brightness, diminishing gradually towards the outer edges. The galaxy appears to have a subtle disc. There is no evidence of strong spiral arm structure or significant dust lanes. No major disturbances in the shape or prominent merging features are discernible. The galaxy exhibits a color gradient, with the central regions appearing slightly redder compared to the bluer outer regions. This color difference indicates potentially older stellar populations concentrated towards the center. Star formation rates appear to be low.
