The galaxy presents a generally smooth appearance, with a primarily rounded shape. There is some suggestion of internal structure, hinting at possible merging or gravitational interactions. The primary body appears relatively undisturbed, yet there is evidence of disturbances or tidal features in the form of extended and faint light around the main galaxy. This suggests either a minor interaction with a companion galaxy or remnants of a previous major merger. The central region exhibits a slightly yellowish hue, potentially indicative of an older stellar population or dust obscuration, while the outskirts appear bluer, implying younger stars or active star formation. The galaxy is luminous and likely fairly massive.
