The galaxy appears to be a spiral galaxy, with a moderately sized central bulge. The spiral arms are well-defined, tightly wound, and numerous. There is evidence of ongoing star formation within the arms, as indicated by their bluish tint. A bar structure appears to be present, although it may be weak. The galaxy exhibits a generally smooth morphology, with no major signs of interaction or recent merging events, though minor disturbances cannot be ruled out. The disk is not viewed edge-on. The overall ellipticity of the galaxy suggests that it is inclined relative to our line of sight.
