The galaxy presents as a centrally concentrated, elliptical-like structure. The light profile suggests a relatively smooth morphology with a lack of prominent spiral arms or distinct features. The primary color of the central region is a yellow-orange hue, potentially indicating an older stellar population dominated by redder stars. The outer regions appear slightly bluer, suggesting the possibility of some younger stars or ongoing, albeit subdued, star formation. There is no significant distortion or tidal features visible, indicating that it is likely not undergoing a major merger. The galaxy exhibits a moderate degree of ellipticity, appearing somewhat elongated. There are no obvious signs of a prominent dust lane or strong active galactic nucleus activity discernible in the image.
