The galaxy presents a predominantly smooth and concentrated light profile. It appears elliptical in shape, exhibiting a slight elongation. The central region displays a high surface brightness, suggesting a concentrated core or bulge. There is a radial color gradient, with the central region appearing more yellowish-white, transitioning to a reddish hue in the outer regions. This may indicate an older stellar population in the outer regions compared to the center. No distinct spiral arms or prominent dust lanes are apparent. Subtle asymmetries or minor disturbances in the outer regions suggest possible past interactions.
