The galaxy appears as a fairly smooth, centrally concentrated object with a slight elliptical morphology. The core is a bright, yellowish-white, suggesting a population of older stars. There is a faint, diffuse halo surrounding the central region, exhibiting a subtle color gradient transitioning toward redder hues in the outer regions. This reddening could indicate a lower density of younger, bluer stars in the galaxy's outskirts or increased dust extinction. No distinct spiral arm structure or significant dust lanes are discernible. There is a hint of slight tidal disturbance in the outer areas. Overall, the galaxy appears to be relatively undisturbed and exhibits characteristics of a mature system.
