The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. It exhibits a dominant bulge component that appears almost spherical. Color gradients are subtle, with the core region appearing more yellow/orange, suggesting an older stellar population. There are hints of a faint, diffuse halo surrounding the central region, with a fall off of luminosity with respect to radial distance. There is little evidence of active star formation in this region. There do not appear to be any tidal tails or obvious signs of recent major mergers or interactions with other galaxies. The overall morphology suggests a relaxed system, with a somewhat high mass.
