The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated brightness profile, indicative of a dense core. The galaxy displays a nearly circular morphology with only slight deviations from perfect roundness. There is little evidence of significant tidal disturbances or ongoing mergers. The color appears generally uniform across the galaxy, showing a subtle shift towards redder hues in the outer regions. The overall structure suggests a system dominated by an older stellar population, with a comparatively low rate of recent star formation.
