The galaxy appears as a moderately inclined disk. It exhibits a central bulge that dominates the overall luminosity. The bulge appears yellow-white, suggesting an older stellar population. Fainter spiral arms are possibly present but are poorly defined. The disk component displays a smoother texture. The galaxy's overall form tends towards a spheroid, but exhibits features indicative of a disk morphology. Evidence of minor gravitational disturbance or interaction cannot be ruled out based on slight irregularities in the disk structure.
