This galaxy presents as a primarily smooth, elliptical-like morphology with a relatively high degree of central concentration. The light distribution suggests a centrally dominant bulge. The overall shape appears to be somewhat rounded, though subtle deviations from perfect sphericity are present. There may be some minor tidal disturbances in the structure of the galaxy. The galaxy exhibits a color gradient, with the core appearing more yellowish-white, transitioning to a bluer hue towards the outer regions. This could be due to a difference in stellar populations. The redder color of the central bulge may indicate an older stellar population, while the bluer regions could contain younger, hotter stars. The overall light profile is indicative of a mature galaxy with a significant stellar mass. Star formation activity appears to be occurring.
