This galaxy presents as a roughly elliptical form with a smooth, diffused light distribution. The central region displays a significantly higher surface brightness, appearing almost spherical and luminous with a yellowish hue. Progressing outwards from the core, the light intensity diminishes gradually. Little evidence exists for any distinct spiral arm structure or prominent dust lanes within the observable extent of the galaxy. Overall, the galaxy's morphology suggests a system dominated by an older stellar population, with low levels of active star formation. There is no obvious signs of tidal disturbances to suggest recent merger activity, and no apparent galactic nucleus.
