The galaxy presents as a relatively smooth, elliptical-like structure. Its morphology indicates a centrally concentrated luminosity profile, with a significant fraction of light emanating from the core. There is little visual evidence of prominent spiral arms or distinct disk features. The overall color appears relatively redder, suggesting a stellar population dominated by older, evolved stars. The roundedness is between round and elliptical. There are no clear signs of tidal disturbances or ongoing major mergers, although minor disturbances cannot be ruled out. 