The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellow-white. The shape is slightly elongated, appearing neither perfectly round nor strongly cigar-shaped. There is no clear evidence of spiral arms or a distinct disk structure. No signs of significant ongoing merging events or major disturbances are visible. The galaxy displays a red-shifted spectrum, indicating a considerable distance. The galaxy appears to be of intermediate mass. There is a relatively low rate of star formation.
