The galaxy presents a face-on orientation, revealing a prominent disk structure. Spiral arms appear moderately defined, with hints of active star formation regions discernible within them. A central bulge is noticeable, contributing significantly to the galaxy's overall luminosity, but does not appear to dominate the disk component. The galaxy exhibits a color gradient, shifting from bluer hues in the outer spiral arms to yellower tones towards the central bulge. The galaxy appears somewhat disturbed, with subtle asymmetries potentially indicating an ongoing or past interaction with another galaxy. There is no apparent strong bar structure.
