The galaxy presents a predominantly smooth morphology. It exhibits an elongated shape, appearing cigar-shaped when viewed from our perspective. There's a concentration of light toward the center, suggesting a bulge. The color distribution appears to show a redder hue in the central regions, likely indicating an older stellar population, while the outer regions exhibit bluer tints. The galaxy does not show any strong signatures of ongoing mergers or major disturbances, though subtle asymmetries cannot be ruled out.
