The galaxy presents as a spiral structure, with a notable central bulge. The arms appear somewhat tightly wound, indicative of a possibly more evolved spiral galaxy. There appears to be a relatively smooth and extended disk component. The color profile suggests the presence of both older stellar populations in the bulge and ongoing star formation, as indicated by the slight bluer hue of the disk. Evidence suggests it may have a bar structure, a stellar bar runs through the center of the galaxy. There also seem to be traces of minor disturbances.
