The galaxy appears to be a spiral galaxy, possibly of the Sa or Sb type, seen at a moderate inclination. It has a bright, concentrated central bulge that dominates the overall luminosity. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population with lower ongoing star formation. 

Faint spiral arms extend from the bulge, showing a bluer color, indicating the presence of younger, hotter stars and regions of active star formation. The arms are somewhat flocculent and less well-defined, suggesting a possibly disturbed or undergoing a period of interaction. There is an indication of a possible tidal tail or minor disturbance on one side of the galaxy. Overall, the galaxy shows a notable amount of light, consistent with an actively star-forming galaxy.
