This galaxy presents as a relatively smooth, centrally concentrated structure. The overall morphology appears elliptical, lacking any distinct spiral arm features or prominent disk-like structure. A significant amount of light is emitted from its core, indicating a dense stellar population or active galactic nucleus. A very faint blueish halo surrounds the core, indicating recent star formation is occuring, but at a low rate. There does not appear to be any evidence of a major ongoing merger or significant tidal disturbance, although subtle asymmetries might be present upon closer inspection.
