The galaxy presents as an elongated, cigar-shaped structure with a noticeable central bulge. The color gradient transitions from a yellowish core to fainter, bluer hues in the outer regions, which suggests a distribution of stellar populations where older stars are concentrated in the center and younger stars may be forming in the disk. The disk appears relatively smooth with no clear spiral arm structures. There are possible indications of a very minor disturbance. Overall, the galaxy's morphology points towards an early-type spiral or lenticular galaxy undergoing relatively low levels of star formation.
