The galaxy presents as a spiral type, viewed at an angle oblique to face-on. Distinct spiral arms are visible, though somewhat flocculent in appearance, tracing an open morphology. The central bulge exhibits a moderate size relative to the overall disk. Indications suggest a weak bar structure may be present within the central region. The disk demonstrates clumpy regions, potentially associated with ongoing star formation. Evidences suggest this galaxy has likely undergone a merger process in its past, or is in the process of one now, due to signs of disturbance.
