The galaxy appears as a centrally concentrated, elliptical-like structure. Its light distribution seems relatively smooth, lacking prominent spiral arms or strong dust lanes. The central region exhibits a yellowish hue, suggesting an older stellar population. The outer regions appear fainter and slightly bluer in color, possibly indicative of some younger stars. There is little evidence of major disturbances, such as tidal tails or asymmetric features, indicating a relatively quiescent state. The overall structure suggests it's likely a massive galaxy with a significant bulge component.
