The object appears to be a galaxy, exhibiting a roughly elliptical morphology. The central region displays a concentrated brightness, with a yellowish-green hue, possibly indicating an older stellar population or significant dust obscuration. Surrounding this central concentration is a bluer ring, implying a region of more active star formation. 

There is evidence of some disruption or tidal features, with a faint, diffuse extension visible that may indicate a possible minor merger event or gravitational disturbance. However, the bulk of the galaxy appears relatively undisturbed. The overall color gradients suggest a complex stellar population and star formation history.
