The galaxy presents as an elongated structure, visually appearing cigar-shaped. The central region exhibits a concentrated, smooth distribution of light, with a color gradient trending towards warmer hues in the core. The outer regions, while less defined, show some hints of cooler color components, possibly indicating areas of ongoing star formation or the presence of a disk-like structure. There does not appear to be any major disturbance of the galaxy, such as a recent merger.
