The galaxy presents as a spiral galaxy with a prominent disk structure. The disk is oriented at a noticeable angle relative to the observer's line of sight. Two spiral arms are visibly emanating from the central region of the galaxy, exhibiting a relatively tight winding pattern. The central bulge appears significant, constituting a moderate fraction of the galaxy's overall brightness. A distinct bar structure appears to bisect the central bulge, oriented along the major axis of the galaxy, the bar's presence is strong. The galaxy's morphology doesn't suggest any on going major merger events or major disturbances, however, the is minor disturbance. No indications of a dominant or negligible bulge size are visually apparent.
