The galaxy presents a largely smooth, elliptical morphology. There is little evidence of distinct spiral arms or a prominent disk structure. The light profile appears centrally concentrated, with a gradual decrease in surface brightness outwards from the core. The central region exhibits a yellowish-orange hue, which could indicate an older stellar population and a lower rate of ongoing star formation. Fainter, more diffuse light extends outwards, with subtle blue tinges, potentially suggesting regions of more recent, but subdued, star formation. There's no apparent major disturbance to the overall structure, but there are subtle asymmetries in the outer regions, perhaps indicative of past minor interactions. The general roundness of the galaxy indicates a relatively evolved system that has likely undergone significant dynamical relaxation.
