The galaxy presents a generally smooth, elliptical morphology. There is a central concentration of light that appears more reddish, possibly indicating an older stellar population within the galactic nucleus. Extending outward from this central region, the galaxy exhibits a diffuse, bluish halo. The lack of clearly defined spiral arms or distinct features suggests that star formation is relatively quiescent. Overall, the galaxy appears to be an evolved system, consistent with an elliptical classification and low star formation rate.
