The galaxy presents as a generally smooth, centrally concentrated object. The core region exhibits a high degree of luminosity, appearing nearly spherical and bright yellow-white in color. Moving outward from the core, the intensity of light gradually decreases into a fainter, more diffuse halo. The overall shape transitions from round to an elongated, elliptical form. There is a very subtle suggestion of disk-like structure extending away from the central bulge, but these features are faint. The object shows little evidence of major disturbances or ongoing merging activity, but some minor irregularities cannot be ruled out at this resolution. The color gradient suggests older stellar populations dominate the central region, and the outer regions may contain a small number of younger, bluer stars. Star formation appears to be low, and this object may represent a relatively evolved system.
