The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The light profile suggests a relatively old stellar population, with a dominant yellowish-orange hue. The galaxy appears largely featureless, lacking any distinct spiral arms or prominent dust lanes. There is a slight elongation, deviating from a perfectly circular shape. The overall structure appears relaxed, with no obvious signs of recent or ongoing major mergers or tidal disturbances. Faint, diffuse light extends outwards from the central region, gradually fading into the background.
