The galaxy presents as a spiral type, exhibiting distinct, though somewhat tightly wound, spiral arms. The central bulge is moderately sized and shows a relatively bright intensity, with a clear concentration of light towards the galactic nucleus.  The disk component appears relatively smooth and the ellipticity suggests a moderate inclination relative to our line of sight.  There appears to be a weak bar structure present, contributing to the arm morphology. There is no obvious major distortion indicating a recent major merger, but some minor disturbances may be present given the irregular structure of the spiral arms.
