The galaxy presents as a spiral galaxy viewed edge-on. A prominent central bulge dominates the structure, appearing significantly brighter than the surrounding disk. The bulge exhibits a rounded shape, indicative of a classical bulge morphology. The disk component is thin and elongated, characterized by a smooth, diffused light distribution. There is no apparent dust lane. No signs of any merging activity or morphological disturbances are observed. The galaxy shows relatively low ongoing star formation.
