The galaxy presents as a relatively small, disk-shaped object. Its central region exhibits a bright, bluish-white hue, which might indicate a high concentration of young, hot stars or significant ongoing star formation. There appears to be some patchy, darker material silhouetted against the blue emission, possibly dust lanes. The outer regions of the galaxy fade in intensity. The overall smoothness indicates a relatively evolved system that is not undergoing any major disruptive processes. It is not perfectly smooth though, and there may be signs of tidal disturbances.