The galaxy presents as an elliptical morphology, though not perfectly spherical. It appears to be mostly smooth in texture and structure. The central region exhibits a concentrated brightness, fading gradually outwards. The color gradient suggests a relatively evolved stellar population, with a yellowish hue concentrated towards the center and a slightly bluer tinge in the outer regions, which could indicate the presence of some younger stars or dust. There is no strong evidence of spiral arms or a distinct disk structure. There is a slight hint of tidal disturbance in the form of a faint extended structure, possibly indicating a past minor interaction or merger. No strong signs of active galactic nuclei are apparent.
