The galaxy exhibits a somewhat irregular spiral morphology. The spiral arms are visible, though not tightly wound. There is evidence of a bar structure bisecting the central region. The bulge appears relatively small, with much of the overall brightness emanating from the disk. Blue and white colors are predominant, suggestive of a significant population of younger stars. There might be some minor tidal disturbances visible along the outer edges of the galaxy, possibly indicating past interactions or mergers. The galaxy appears to be at a moderate inclination relative to our line of sight.
