The galaxy presents as a disk galaxy, seen edge-on. There is a bright, concentrated central bulge, which appears relatively smooth in texture. A flattened disk extends outward from the bulge, appearing elongated due to the edge-on viewing angle. The disk exhibits a yellowish hue, potentially indicative of an older stellar population. The high fraction of observers who considered this galaxy to be edge on suggests a consistent morphological interpretation. There are some hints of a possible minor disturbance or interaction, as suggested by the high number of observers who noticed merger activity.
