The galaxy presents as a somewhat elongated, irregular object with a central, more concentrated region. This core exhibits a yellowish-orange hue, possibly indicating an older stellar population or dust obscuration. Surrounding this central area is a bluer halo, suggesting the presence of younger, hotter stars and potentially ongoing star formation. 

The galaxy displays some structural features, but these are not clearly defined spiral arms or a distinct disk. There is a slight elongation visible, and the galaxy appears to have a mild disturbance or asymmetry in its morphology, with one side appearing slightly more extended or disrupted than the other. The overall impression is of a galaxy that is either in the process of formation or has undergone some interaction that has disturbed its morphology.
