The galaxy appears to be a spiral galaxy, viewed at an oblique angle. The central bulge is prominent and appears yellowish-white, possibly indicating an older stellar population with less active star formation in that region. A flattened disk is visible, but the spiral arms are not sharply defined; they appear somewhat diffuse and patchy. Some minor disturbances may be present, given the slightly irregular shape of the galaxy. The overall color suggests a mix of stellar populations, with some regions possibly exhibiting ongoing, albeit not vigorous, star formation. It exhibits a relatively compact structure and medium mass range. 
