This galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an elliptical morphology, appearing mostly rounded, with subtle deviations from perfect sphericity. No distinct spiral arm structure or significant dust lanes are visible. The color profile suggests a population of older stars, with a hint of bluer light potentially indicating some recent star formation. There might be a very minor disturbance present, but overall, the galaxy appears to be relatively undisturbed. The mass is fairly average. The star formation rate appears to be quite low for the mass present.
