The galaxy presents as a face-on spiral galaxy with a pronounced central bar structure. The spiral arms are easily discernible and loosely wound. The disk is not perfectly symmetrical, exhibiting a slightly irregular shape, potentially indicating a recent interaction or minor disturbance. The central bulge appears relatively small compared to the disk size. Active star formation regions are suggested within the spiral arms, observed as brighter, somewhat bluer knots throughout the disk. There is the appearance of two faint tidal tails extending from the galaxy, indicating an interaction with another galaxy.
