The galaxy appears to be an elliptical, with a largely smooth light distribution. The core is bright, with a gradual decrease in luminosity towards the edges. The overall shape is roughly circular but not perfectly so. There is no discernible spiral arm structure or a prominent disk component; it would appear to be a spheroidal galaxy, exhibiting an old stellar population with little to no current star formation activity. The red color may support that. There is no evidence of recent major mergers or significant tidal disturbances.
