The galaxy presents as a centrally concentrated object with a generally smooth morphology. The dominant light profile suggests a relatively featureless structure, potentially elliptical or lenticular. The central region exhibits a yellowish-orange hue, suggestive of an older stellar population, while the outer regions appear slightly greener. The faint green coloration suggests the presence of ongoing, albeit potentially low-level, star formation, at least compared to the core of the galaxy. There is no visually discernible presence of strong tidal features or a prominent disk structure.
