The galaxy presents as a somewhat elongated, cigar-shaped structure. It appears to be a relatively smooth galaxy, exhibiting a diffuse, hazy morphology without prominent spiral arms or a distinct central bulge. The color profile suggests a mix of stellar populations; a central yellowish-green hue likely indicates the presence of older stars, while the fainter bluish-white regions suggest the presence of younger, hotter stars within the galaxy. There is a hint of possible minor disturbances or tidal features, but the overall morphology points more towards a quiescent system. It appears to be a galaxy with a mass estimate around 10^10 solar masses, and a possible star formation rate around 10^0 solar masses per year. 
