The galaxy presents as a roughly circular structure, with a notable concentration of light towards its center. The core region exhibits a yellowish hue, possibly indicating an older stellar population. Extending outwards from the core is a fainter, bluer halo. There appears to be some irregularity in the outer regions of the galaxy, suggesting possible gravitational interaction or ongoing merger activity. The overall impression is of a galaxy undergoing some form of dynamic process affecting its morphology.
