The galaxy presents an elliptical morphology with a smooth light distribution. Its central region exhibits a high concentration of light, appearing bright and yellowish-orange. This suggests an older stellar population dominating the core, possibly with ongoing low-level star formation. The outer regions of the galaxy are less defined and fainter, fading gradually into the background. There is a faint, irregular bluish extension or tidal feature on one side, which may suggest a minor interaction or accretion event. The overall color profile implies a galaxy that has largely ceased active star formation, though some residual activity might be occurring. It appears as a relatively undisturbed system with a dominant bulge.
