The galaxy presents as a spiral type, exhibiting well-defined spiral arms that emanate from a central bulge. The arms appear to be wound moderately tightly, with some exhibiting a flocculent or patchy structure, indicating regions of active star formation. The galaxy's disk is inclined relative to our line of sight, not perfectly edge-on, but visibly tilted. The central bulge region displays a relatively smooth and concentrated appearance. The galaxy shows signs of weak to no bar structure across the central part of the bulge. There are not any signs of major mergers or disturbances. The galaxy has a bluer tint, suggesting some young stellar populations.
