The galaxy exhibits a prominent spiral structure. Its disk is viewed at an angle, but is not completely edge-on. Evident are spiral arms extending outwards from the central region, with hints of tightly wound morphology. The galaxy appears to be undergoing an interaction with a smaller companion object, characterized by signs of tidal disturbances or merging activity that may be disrupting its structure. A moderate bulge is present within the galaxy's center. The disk is a mixture of faint blue and white starlight.
