The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color appears to be on the redder side, suggesting an older stellar population. There is a bright central bulge, which is the most luminous region of the galaxy. The galaxy's shape is elongated, and the light distribution is relatively uniform without any prominent spiral arms or distinct features. There is no visible dust lane or evidence of active star formation regions. The galaxy appears isolated, with no apparent signs of tidal interactions or ongoing mergers with other galaxies.
