This galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent bulge is visible at the galaxy's center, appearing relatively smooth and bright, suggesting a concentration of older stars. The disk component, extending outwards from the bulge, is visible with slightly bluer hues, indicating the presence of younger stars and potentially ongoing star formation. There are no obvious signs of strong spiral arm structure or significant dust lanes that would normally obscure the light from the stellar population. The overall morphology shows no signs of any recent mergers, though the disk may exhibit some minor disturbances.
