The galaxy appears to be a disk galaxy viewed at a significant angle, approaching edge-on, as evidenced by its elongated shape. There is a prominent bulge, possibly a classical bulge, that is fairly large and concentrated. The light distribution suggests a higher concentration of older stars in the bulge, characterized by yellow and orange hues. The disk component is less prominent and shows hints of bluer regions, suggesting on-going star formation. The galaxy appears to have a relatively smooth overall appearance. There is little indication of strong tidal interactions or major mergers, although minor asymmetries are present. The colours suggest a mix of stellar populations, with a dominant older population and a younger population in the disk. The red shift indicates that this is a fairly distant galaxy.