The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The light profile appears uniformly distributed without prominent spiral arms or distinct morphological features. Its shape is distinctly round. The color gradient suggests an older stellar population, appearing reddish-yellow, with no strong evidence of ongoing, active star formation regions. There is a possible indication of a minor disturbance in the galaxy’s form, though it appears to be relatively undisturbed.
