The galaxy appears as a relatively small, elliptical or lenticular-shaped structure with a centrally concentrated bulge. There is a noticeable color gradient, shifting from bluish tones at the outer edges of the galaxy to reddish hues in the central region. This color variation could indicate differing stellar populations, with younger, hotter stars dominating the outer regions, and older, cooler stars concentrated toward the center. There may be a slight hint of a disk-like structure, although it is not prominently defined. There is some evidence of tidal disruption or gravitational interaction. It is possible the light from the galaxy is contaminated by artifacts. 