The galaxy presents as a spiral type, viewed at a moderate inclination, not quite face-on. Two distinct spiral arms are readily apparent, exhibiting a relatively tight winding pattern. Star forming regions appear to be present, as suggested by the clumpy texture of the arms and slightly bluer color than the bulge. The central bulge appears moderately sized and luminous, indicating a considerable stellar population. A weak bar structure might be present across the nucleus of the galaxy. Overall, the galaxy appears relatively undisturbed, with no strong signs of major mergers. There may be a minor disturbance or tidal debris on one side.
