The galaxy presents as a moderately bright, elliptical system. It exhibits a relatively smooth morphology with no prominent spiral arm structures or bar features readily apparent. The core region appears concentrated, with a gradual decrease in luminosity towards the outer regions. There is a slight elongation, deviating from a perfect circular shape. The galaxy's color profile suggests a redder hue, likely indicative of an older stellar population. The overall structure seems undisturbed, with no major signs of ongoing mergers or tidal interactions, though a slight asymmetry cannot be ruled out.
