The galaxy presents as an elongated, disk-like structure with a noticeable central bulge. The central region is bright, appearing relatively smooth and concentrated. Surrounding this bulge, a fainter, more diffuse disk extends outwards. The disk appears to have some features present in the image suggesting it is a spiral galaxy. The galaxy exhibits a blueish hue, suggestive of ongoing star formation within the galaxy, though this is primarily concentrated toward the center. The outer regions of the disk show hints of spiral arm structure, but appear rather faint and dispersed. Overall, the galaxy exhibits a moderate degree of smoothness, but shows some indications of internal structure. The galaxy seems to be an isolated system.
