The galaxy presents a largely smooth and rounded morphology, appearing nearly circular in projection. A bright, concentrated central bulge dominates the structure, emitting strongly in the green and blue wavelengths, suggesting a significant population of relatively young, hot stars in this region. The outer regions exhibit a more diffuse and less defined structure, with hints of spiral arm-like features. The overall color appears slightly blue, indicative of ongoing star formation, although the bulge appears to be older. There is no obvious evidence of major mergers or significant tidal disturbances in the immediate vicinity, though there seems to be a slight irregularity on one side of the galaxy. The galaxy shows a substantial amount of light as it is very luminous.
