The galaxy presents as a singular, fairly symmetrical object with a smooth, elliptical morphology. The light distribution appears concentrated towards the center, exhibiting a bright, almost uniform core. The outer regions fade gradually into the background, showing a diffuse halo. There is minimal evidence of any prominent spiral arms or distinct features such as dust lanes or knots of star formation regions, consistent with a relatively quiescent state. The color profile suggests an older stellar population, the overall color leaning towards redder wavelengths. Any signs of recent or ongoing mergers are not visible.
