The galaxy presents as a spiral with a notable disk structure. The spiral arms are prominent, showing a relatively open winding. Some disruption is seen in the spiral arm morphology. The central bulge is moderately sized. It is not clear whether there is a central bar or not.

The galaxy exhibits a range of colors, with the bulge showing a yellower hue, suggestive of an older stellar population. The disk and spiral arms show bluer tints, indicative of younger, hotter stars and ongoing star formation. The overall structure suggests the possibility of a minor disturbance due to an interaction.
