The galaxy exhibits an elongated, cigar-shaped morphology, suggestive of an elliptical galaxy. The central region displays a bright, concentrated core exhibiting a yellowish hue, likely indicative of an older stellar population. Moving outward from the core, the light gradually diminishes, transitioning into a fainter, bluer halo. The outer regions display a disk like structure, but are still quite smooth. No distinct spiral arms or prominent dust lanes are discernible. The overall smoothness of the galaxy suggests it is not currently undergoing a major merging event, though there might be a slight disturbance or recent minor merger. 
