This galaxy presents as a relatively smooth, elliptical or lenticular-like structure. It exhibits a concentrated central bulge that gradually fades into the outer regions of the galaxy. The color profile suggests a generally older stellar population, with a yellow to red hue concentrated in the central region, indicating a lack of significant recent star formation. The galaxy appears largely undisturbed, with no obvious signs of major merger events or tidal distortions. A small hint of a possible disk is seen, but it seems to be mostly spheroidal in nature. No distinct spiral arms are seen.
