The galaxy appears as a diffuse, centrally concentrated object. The core exhibits a bright, yellow-orange hue, possibly indicative of an older stellar population or dust obscuration. Extending outward from the core is a less luminous, blue-ish halo. This suggests the presence of a younger stellar population perhaps undergoing active star formation. The outer regions seem somewhat irregular, possibly indicating gravitational interactions or past merger events disrupting its overall structure. There's also the suggestion of faint tidal features or plumes emanating from the main body, further supporting a history of dynamical interaction. The galaxy does not appear to have a clearly defined spiral structure or a smooth elliptical profile.
