The galaxy appears to be an elliptical, cigar-shaped galaxy with a smooth profile and no apparent spiral arm structure. It presents a concentrated central bulge that is very bright and emits a yellowish light, possibly indicating an older stellar population. The overall color appears to be on the redder side, which correlates to an older stellar population that is not experiencing high rates of star formation. There is no dust lane visible. Given its overall morphology and color, this galaxy likely has a high mass and a very low specific star formation rate. There is no evidence of any ongoing or recent major mergers. The outer regions of the galaxy fade smoothly into the background sky.