The galaxy presents as a somewhat elliptical structure, with a moderate degree of elongation. The overall color profile appears generally redder, suggesting an older stellar population. There is a high degree of smoothness, with no discernible spiral arms or distinct features within the visible disk. The concentration of light increases significantly toward the center, culminating in a bright, compact core. There is a potential minor tidal disturbance, which is suggested by a faint asymmetrical feature around the galaxy's center.
