The galaxy presents a complex morphology, appearing to be in a state of interaction or disturbance. The primary component exhibits a generally rounded shape, with a diffuse, less defined outer structure. There are faint indications of tidal features or extensions emanating from the main body, especially towards the lower portion, suggesting gravitational interactions with another galaxy or object.

The color profile indicates a population of stars with intermediate ages. The central region shows a bluer hue, possibly indicative of recent or ongoing star formation. The outer regions appear redder, suggesting the presence of older stellar populations or dust obscuration.

Overall, the galaxy's visual characteristics point towards a system undergoing significant dynamical processes. Evidence for merger activity or strong gravitational interactions is prominent, which may be contributing to the observed enhanced star formation in the central regions. The system presents a departure from a quiescent, well-defined spiral or elliptical morphology.
