The galaxy presents as a somewhat elliptical, disk-like structure with a central bulge. The bulge appears smooth and concentrated, exhibiting a yellowish hue, suggesting a population of older stars. The disk, while discernible, is not sharply defined and shows a fainter, bluer color indicative of younger stars and potential star formation regions. One side of the galaxy seems to have a more diffuse and extended structure compared to the other, with possible signs of tidal features or minor disturbances. Overall, it looks like a relatively isolated galaxy with no major merger events actively occurring, but with indications of potential past interactions.
