The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellow-orange hue, suggesting an older stellar population with a low rate of current star formation. The galaxy appears to be fairly round in shape, without significant distortions or tidal features indicating major ongoing merger activity. There are hints of some minor structural disturbances. Based on its color and morphology, this galaxy is likely a massive system, with a significant number of stars.
