This galaxy presents as a primarily smooth object with a slight elongation, trending towards a cigar shape. It shows a central bulge that appears brighter and more condensed than the surrounding galactic disk. A faint, diffuse disk extends outwards from the central bulge. There is some subtle evidence of spiral arm structure within the disk, although they appear tightly wound and are not sharply defined. The galaxy exhibits a predominantly blue hue, hinting at ongoing star formation. There are no obvious signs of a major ongoing merger, although there may be some minor disturbances in the galactic structure. Overall, this galaxy appears as a relatively undisturbed spiral galaxy, likely observed at a moderate distance.
