The galaxy presents as a grand design spiral, viewed at an angle slightly offset from face-on. Two prominent spiral arms emanate from a central bulge region. These arms display a relatively open winding pattern. The central bulge appears yellowish, suggesting an older stellar population, while the spiral arms exhibit a bluer hue, possibly indicative of ongoing star formation. No significant tidal distortions or signs of major mergers are immediately apparent, though a minor disturbance cannot be ruled out. A bar feature appears to be present, bisecting the bulge, which may be classified as strong to weak in strength. The bulge size appears to be small to moderate, with spiral arms clearly dominating the galactic structure.
