The galaxy exhibits a smooth, elongated morphology, resembling a cigar shape. There is little evidence of distinct spiral arms or significant disk-like features; it appears largely featureless. The light distribution suggests a centrally concentrated structure with a gradual decrease in luminosity toward the outer regions. No prominent dust lanes or active star-forming regions are readily apparent. The overall color appears relatively uniform, with a subtle blue tint to it. There is no indication of a major ongoing merger event, although there is a hint of some minor interaction or disturbance to the galaxy. 
