The galaxy appears to be a spiral type, viewed at a slight angle, not quite face-on. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. Spiral arms are discernible, although not sharply defined. These arms display a mix of bluish and yellowish regions, hinting at both recent star formation and older star clusters. The spiral arms appear somewhat tightly wound around the bulge. There is a suggestion of a bar-like structure crossing the central bulge. The disk of the galaxy is relatively thin, but not fully edge on. There appear to be 2 or 3 main spiral arms that seem to branch off from the center. There is no evidence of a major merger event, though a possible minor tidal interaction is visible. Overall, the galaxy appears to be a moderately massive, actively star-forming spiral galaxy at a considerable distance.
