The galaxy presents a generally smooth appearance, with a discernible elliptical morphology. The light distribution suggests a central bulge, surrounded by a more diffuse halo. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a redder periphery. This color variation is suggestive of older stellar populations dominating the outer regions, while younger, hotter stars are concentrated within the central region. There is some indication of minor disturbances in the morphology, possibly due to tidal interactions or internal processes. The galaxy's overall structure suggests it is likely a relatively massive system that is not forming stars very actively. 
