The galaxy presents a clear edge-on morphology, exhibiting a flattened, cigar-like shape. A central bulge is visible, characterized by a yellowish-white hue, indicating a likely population of older stars. Fainter bluish regions appear at the outer edges of the galaxy. This might suggest the presence of ongoing star formation within the galactic disk. The galaxy appears relatively undisturbed, without any obvious signs of a major merger or tidal disruptions, suggesting a relatively isolated evolutionary path. A small amount of asymmetry is observed. 
