The galaxy presents a somewhat elongated, cigar-shaped morphology. It exhibits a central bulge that appears relatively smooth and concentrated, transitioning into a disk-like structure. There is evidence of possible spiral arm features, though they are not sharply defined. These features are bluer in color, suggesting areas of younger stellar populations, while the central bulge has a more yellowish hue, potentially indicating older stars. The galaxy does not appear to be undergoing any major merging activity, although there may be some minor distortions in the outer disk. Overall, the galaxy seems to be a relatively massive system, with signs of moderate star formation.
