The observed galaxy exhibits a clear spiral structure. The spiral arms are well-defined and extend outwards from a central bulge. The arms appear grand design. There are hints of faint spiral arms and a substantial disk. A small, bright core is visible, indicative of a possible active galactic nucleus. The galaxy appears relatively undisturbed, without significant signs of tidal interactions or major mergers. There may be a weak bar structure. The galaxy has a moderate amount of star formation throughout.
