The galaxy presents as a disk-shaped system, viewed at a high inclination. The galaxy exhibits a pronounced central bulge, appearing bright and concentrated. The disk component appears to be a mixture of smooth, diffuse light. The system is approximately 12 kpc in radius and exhibits a low star formation rate. The galaxy is estimated to have a stellar mass slightly over 10^11 solar masses. There is no apparent signs of any major merging activity or tidal disturbances visible in this image.
