This galaxy presents as a spiral type, viewed at a slight angle from face-on. It exhibits a well-defined, though not particularly prominent, central bulge. The spiral arms appear somewhat tightly wound, predominantly featuring two distinct arms. The color distribution suggests active star formation regions, with a bluer hue concentrated along the spiral arms, contrasted by a yellower central bulge which may indicate an older stellar population. No significant disturbances or signs of ongoing mergers are readily apparent, though some asymmetry in the outer regions suggests past interactions cannot be ruled out. There may be a faint bar structure crossing the center. Overall, the galaxy appears to be a relatively normal spiral galaxy undergoing moderate star formation.
