The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a centrally concentrated light profile. The core region displays a bright, slightly bluish-white hue, suggesting the presence of a population of younger, hotter stars and potentially ongoing star formation, albeit at a low rate. There appears to be a subtle color gradient moving outward from the center, with the outer regions exhibiting a more yellow/reddish tint. This indicates an older stellar population in the outskirts. No distinct spiral arm structures or prominent dust lanes are discernible, supporting the classification as a relatively undisturbed system with no major ongoing merger activity. The overall shape appears more in-between rounded and elliptical than strongly elongated. The galaxy is relatively compact in size, but its high absolute magnitude suggests a substantial stellar mass.
