The galaxy presents a relatively smooth and symmetrical morphology. The central bulge is prominent, exhibiting a yellowish-red hue, suggestive of an older stellar population. Surrounding the bulge is a more diffuse, bluish halo. This halo appears somewhat elongated, though the galaxy does not exhibit a clear spiral structure, indicating it is likely an elliptical galaxy. There is a slight hint of irregular structure, which could indicate some recent interaction. Overall, the galaxy appears to be relatively isolated, with no signs of major tidal disturbances or ongoing mergers.
