This galaxy presents a somewhat elongated, cigar-shaped morphology. A smooth, centrally concentrated bulge dominates the overall structure, emitting light that appears predominantly white with a slight bluish tint. Fainter, bluer, diffuse emission extends outward from the central bulge in a flattened, disk-like structure, suggesting the presence of younger stars or ongoing star formation. The outer edges of the disk appear indistinct and somewhat irregular. There is no clear evidence of spiral arms or a well-defined dust lane within the visible portion of this galaxy. It does not show any signs of an ongoing merger, although there appears to be some minor disturbance of it's disk.
