This appears to be a spiral galaxy, seen at an oblique angle. A central bulge is clearly visible, exhibiting a yellowish-orange hue. The spiral arms are tightly wound around the bulge. The galaxy appears to have at least 3 distinct arms, though they are not very clear due to the image quality and distance. Some of the arms seem to have bluer tinges suggesting the presence of active star formation regions. The lack of significant tidal distortion suggests that it is not undergoing a major merger event. There is no evidence of a strong bar feature. The overall appearance suggests a galaxy dominated by older stellar populations in the bulge, with ongoing star formation predominantly within the spiral arms. The galaxy is likely of moderate mass and experiencing moderate star formation.
