The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light profile suggests a relatively even distribution of stars with a noticeable concentration towards the galactic nucleus. There are no apparent spiral arm structures or significant dust lane features. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a slightly bluer halo. This suggests a population of older stars concentrated in the center, with a slightly younger stellar population in the outer regions. Overall, the galaxy appears largely undisturbed, with no evidence of major mergers or significant tidal interactions.
