The galaxy presents as a largely featureless elliptical, with a smooth, concentrated light profile that diminishes radially. The core region shows a bright, yellowish-white hue indicative of an older stellar population. There is little evidence of distinct spiral arms, dust lanes, or regions of active star formation. The overall shape is close to circular, exhibiting a high degree of symmetry. Slight hints of a more diffuse halo are present, extending subtly beyond the main body of the galaxy. No signs of tidal tails or ongoing merger activity are readily apparent. The galaxy appears relatively isolated and undisturbed.
