The galaxy presents as a luminous, elliptical-shaped structure. Its core exhibits a bright, concentrated glow that diminishes in intensity towards the outer edges. The light distribution appears relatively smooth and uniform, lacking the prominent spiral arm features typically associated with disk galaxies. The overall color profile seems to be slightly skewed toward the redder end of the spectrum. The morphology suggests that it is likely a fairly massive galaxy with a moderate star formation rate. No obvious signs of ongoing merger activity or significant tidal disturbances are readily apparent.
