The galaxy presents as a relatively smooth, elliptical-like object. Its color profile suggests an older stellar population, with a noticeable concentration of light towards the center. The galaxy appears mostly featureless, lacking prominent spiral arms or distinct dust lanes. It exhibits a subtle elongation, deviating slightly from a perfectly circular shape. There is no obvious evidence of active galactic nuclei activity or ongoing major merging events. The galaxy's overall morphology indicates a system dominated by stars with minimal ongoing star formation.
