The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. Its color profile suggests an older stellar population, exhibiting a yellowish-red hue in the central regions, likely indicative of evolved stars. A subtle greenish tint surrounds the central bulge. There is minimal indication of spiral arms or significant dust lanes within the visible spectrum of this image. The galaxy appears relatively undisturbed, showing no obvious signs of ongoing major merger activity or tidal distortions. The overall morphology is consistent with an early-type galaxy, and it is approximately 4.6 Kpc in diameter.