The galaxy presents a primarily smooth morphology, with an elliptical appearance. The concentration of light suggests a prominent bulge component. The galaxy exhibits a dominant yellow-orange color, suggestive of an older stellar population. There is slight evidence of bluer regions indicating the presence of some younger, hotter stars, but they appear subdued, indicating low ongoing star formation. The shape appears to be somewhere in between round and oblong. There is no visible signs of any major disturbances in the symmetry of the galaxy and no indications of any tidal features or close companions that would suggest an ongoing or recent merger event. 
