The galaxy presents a generally smooth morphology, with the light concentrated towards the central region. The isophotes are relatively regular and elliptical in shape. The central region exhibits a yellowish-white hue, suggesting an older stellar population dominating the core. The outer regions transition to a bluer tint, indicating the presence of younger, hotter stars, although to a lesser degree than the central region. Overall, the galaxy appears to be a relatively isolated system, showing no major signs of ongoing mergers or significant tidal disturbances. The light profile indicates a relatively high concentration of stellar mass in the galactic center.
