This galaxy presents as a relatively smooth and featureless object. The light profile appears centrally concentrated, displaying a high degree of radial symmetry. Its shape is noticeably elliptical, trending toward a more rounded, though not perfectly spherical, morphology. There is no clear evidence of a spiral arm structure or strong tidal features, suggesting minimal recent major merger activity. The color gradient indicates a redder core region surrounded by a bluer halo. This color difference implies the presence of an older stellar population in the galactic center, while younger, hotter stars may be more prevalent in the outer regions. Minor disturbances may be present, however it is likely that there is not a current merger event. Based on these observations, the galaxy can be characterized as an elliptical galaxy exhibiting signs of relatively low levels of star formation and is moderately massive.
