The galaxy presents as a spiral, with two prominent arms visible. The arms are not tightly wound, rather they appear to be moderately spread. The morphology suggests the galaxy is not undergoing any major merger activity, though there is some slight asymmetry. A bar-like structure appears to cut through the central bulge. The bulge itself is relatively small compared to the overall size of the galaxy, although it shows signs of extended diffuse light. The overall color of the galaxy is fairly red, suggesting a relatively older stellar population, and the presence of more dust. The redder colour could also be affected by redshift. The disk dominates the galaxy's morphology, showing features attributable to ongoing star formation.
