The galaxy exhibits a generally elongated, cigar-like morphology. It appears relatively smooth in overall texture, though there is a subtle hint of internal structure. The galaxy shows a central concentration of light, which gradually fades towards the edges, creating a diffuse halo. The color gradient suggests a stellar population with potentially varying ages, with bluer hues possibly indicating regions of recent star formation. The red-shifted appearance also suggests that we are observing this galaxy at a significant distance.
