The galaxy presents as a spheroid morphology, likely an elliptical, with a smooth light distribution and a high degree of central concentration. There is some indication of a possible interaction or merger occurring. The shape deviates slightly from being perfectly round; it is closer to in-between round and cigar shaped. There appears to be a secondary, smaller structure in close proximity, hinting at a merging event or tidal disturbance. There is an area that appears slightly more disturbed, but it is difficult to tell the extent of disturbance because of image quality. The color appears to be redder, indicating an older stellar population with a relatively low star formation rate.
