The galaxy presents as a relatively smooth, elliptical-type morphology. It has a centrally concentrated light profile, appearing nearly round in projection on the sky. There are no discernible spiral arms or a prominent disk structure. Faint color variations are subtly present, suggesting an older stellar population. The galaxy exhibits a moderate red shift, indicating that it is at a significant cosmological distance. There is no apparent ongoing major merging activity or tidal disturbance. The galaxy's central core appears somewhat yellow, which may represent an active galactic nucleus or a concentration of older stars. The galaxy has a high mass and a low star formation rate.
