The observed galaxy presents as a spiral galaxy with a relatively bright, moderately sized central bulge. Spiral arms are visible, and appear somewhat patchy and flocculent. The overall color is bluish, suggesting a substantial population of young, hot stars, particularly within the spiral arms. The structure appears slightly disturbed or asymmetrical; possible interactions or tidal features could be present, meriting further investigation. There is no clear evidence of a strong central bar structure. The galaxy is viewed at a slight angle to face-on.
