This galaxy appears to be a spiral galaxy seen nearly edge-on. A prominent central bulge is present, exhibiting a yellowish hue, suggesting a population of older stars. The disk appears thin and elongated, extending outward from the bulge. The disk also has a yellow tint, indicating relatively low ongoing star formation activity. There is no significant dust lane visible, though this could be due to the resolution of the image or the viewing angle. There does not appear to be any merging galaxies or major disturbances. The general morphology suggests a galaxy that is relatively undisturbed, with little interaction with other galaxies. The color suggests that the galaxy has a relatively low star formation rate.
