The galaxy presents as a spiral type, with a relatively large disk extending beyond a moderately sized central bulge. The spiral arms appear well-defined, exhibiting a morphology of two dominant arms. The winding of these arms appears to be of medium tightness. A bar structure is prominently visible bisecting the bulge, although with a moderate strength. The overall color distribution suggests ongoing star formation, with a bluer hue in the disk regions compared to the yellower, redder bulge. No strong signs of tidal disturbances are present. The disk of the galaxy is oriented at an angle that is more face-on rather than edge-on.
