The galaxy appears to be a relatively smooth, elliptical-like structure. There is a concentrated central bulge that is bright and dominates the light output of the galaxy. The galaxy appears to have a slight elongation, presenting an oval shape, leaning towards a cigar shape rather than perfectly circular, but it mostly appears round. There is no apparent spiral arm structure. Color gradients suggest the presence of older stellar populations, possibly indicative of a lower current star formation rate, consistent with ellipticals. There are no visible signs of any major disturbances from mergers or interactions, though a minor asymmetry hints at possible previous interactions.
