The galaxy presents as a flattened, elongated structure, suggesting a disk-like morphology viewed at an oblique angle. The central region exhibits a concentrated, bright luminosity, likely indicating a bulge. The luminosity decreases gradually moving away from the central region into the outer disk. The galaxy appears relatively smooth in texture, with a hint of possible substructure or disturbances in the outer regions of the disk. There is a color gradient visible, with the central bulge appearing more yellowish or gold, and the outer disk exhibiting slightly bluer hues. This suggests the bulge region is populated by older stars and the disk is likely undergoing some active star formation. The overall shape resembles a cigar shape, with an axial ratio suggesting a significant inclination relative to our line of sight. There are no signs of a major ongoing merger.