This galaxy appears to be a relatively smooth, elliptical galaxy. It presents a largely spheroidal morphology with a high degree of central concentration. The light distribution suggests a single component system, with no obvious signs of spiral arms or a disk-like structure. The color gradient appears to be subtly redder towards the central regions, suggesting an older stellar population concentrated in the core. There is no prominent dust lane or any indication of ongoing major merger activity. Faint extensions of the galactic halo may be present but the image resolution limits any definitive statement on this. The observed round shape is indicative of an early-type classification. There is no distinct active galactic nucleus (AGN) visible, as judged from the lack of an overly bright or point-like central source.
