The galaxy presents as a centrally concentrated, generally smooth distribution of light, with an elliptical morphology. The core exhibits a concentration of light, with a falloff in intensity towards the edges. The overall color appears consistent, with an absence of well-defined spiral arm structures or prominent dust lanes. There are hints of minor tidal features or disturbances, and a small chance of an ongoing merger. Given the magnitude, this galaxy is an example of a somewhat massive galaxy with little to no star formation.
