The galaxy presents a morphology consistent with an elliptical galaxy. It exhibits a smooth, diffuse light distribution with a high degree of central concentration. The overall shape appears somewhat elongated, deviating from a perfectly circular profile. The light profile shows a strong concentration towards the center, fading gradually outwards. The color gradient indicates a reddish hue in the central region, transitioning towards slightly bluer tones in the outer parts. This color gradient suggests a stellar population gradient, with older, redder stars dominating the core and a younger, bluer population present in the outer regions, possibly indicating some ongoing or recent star formation. There is no clear evidence of spiral arms or a distinct disk structure. There are no signs of significant tidal disturbances or interactions with other galaxies in the immediate vicinity.
