The galaxy presents as a spiral type, viewed at an angle oblique to face-on, but not quite edge-on. The central bulge appears moderately prominent and exhibits a relatively smooth texture and concentrated light profile.

Spiral arms are visible and well-defined, with a suggestion of flocculent structure. The winding of the spiral arms is moderate. Distinct color variations are present within the arms, implying regions of active star formation interspersed with older stellar populations. The galaxy exhibits indications of minor disturbances, with some asymmetries in its structure. The overall shape is slightly irregular, potentially indicative of past or ongoing interactions.
