The galaxy presents as a disk galaxy, observed at a notable inclination relative to our line of sight, but not edge-on. It exhibits a moderate central bulge. There are indications of a barred structure, with a brighter, elongated region oriented approximately along the major axis of the galaxy. We can see hints of spiral arm structure in the outer regions, though they are not sharply defined. The overall color profile appears to be dominated by older stellar populations, but bluer tinges are present at the end of the bar and in some of the spiral arm regions, indicating potential ongoing star formation in those locations. No signs of major mergers or tidal disturbances are visible, but there may be minor irregularities in the outer disk suggesting some past interaction or accretion event.
