The galaxy presents a predominantly smooth morphology, lacking distinct spiral arms or a prominent central bulge. It exhibits an elongated shape, appearing cigar-shaped in form. The color gradient transitions from a yellowish core to a bluer outer region, suggesting a differential distribution of stellar populations, with potentially older stars concentrated towards the center. There are no obvious signs of a major merger, although there may be minor tidal disturbances or interactions influencing its shape. The smooth appearance indicates that the light emitted from this galaxy is likely from an elliptical system.
