The galaxy presents as a primarily smooth, elliptical object. It exhibits a concentrated central bulge that appears nearly spherical. The color is predominantly yellow, suggesting a population of older stars and a relatively low rate of ongoing star formation. There is no discernable spiral arm structure. There is some evidence of minor disturbances in the galaxy, such as some asymmetry in the outer regions of the halo, though a merger event is unlikely. The galaxy's morphology indicates a relatively high degree of roundness, with minimal deviation from a spherical shape. The galaxy's magnitude suggests that this is a high mass object. 
