The galaxy presents as a relatively smooth, elliptical structure with a bright, concentrated core. The central region exhibits a yellowish hue, suggestive of an older stellar population. Moving outwards from the core, the luminosity gradually decreases, with the outer regions appearing more diffuse and slightly redder in color. There is no discernible spiral arm structure or prominent dust lanes. The overall shape is nearly circular, indicating a low degree of ellipticity. There is no obvious evidence of tidal disturbances or ongoing mergers. The light distribution appears well-fit by a Sersic profile, characteristic of elliptical galaxies.