The galaxy presents as a centrally concentrated, smooth structure with a noticeable colour gradient. The core region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the core, a subtle shift toward a bluish-green colouration is observed, hinting at the presence of younger, hotter stars. The overall form appears somewhat elliptical in shape, and does not show any clear spiral arm structure or significant dust lanes. There is a slight asymmetry, but does not seem to be undergoing a major merger. There is no clear tidal debris or extended halo around the galaxy. The light distribution suggests a system dominated by a bulge with a relatively smooth transition to the outer regions. The object appears relatively undisturbed.
