The galaxy presents a generally smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, transitioning into a broader, diffuse halo. Color gradients are subtle, with a slightly yellower central region that fades into a more neutral hue in the outer regions. No distinct spiral arm structures or significant dust lanes are discernible. There are no apparent signs of ongoing major merger activity or tidal disruptions. The galaxy appears relatively undisturbed, suggestive of a system dominated by an older stellar population with a modest rate of star formation. Its overall appearance suggests it is an early-type galaxy.
