The galaxy exhibits a primarily elliptical morphology, appearing relatively smooth in structure. There's a concentration of light toward the center, suggesting a prominent bulge. Fainter, diffuse features are also visible, possibly indicating a disk component or tidal disturbances, although these are not sharply defined. The galaxy displays a range of colors, with a central region exhibiting a yellowish hue, potentially indicating an older stellar population. Bluer regions are present in the outer parts, which may suggest the presence of younger, hotter stars and ongoing star formation. Based on its colors and shape, the galaxy appears to be an intermediate-mass system. There are hints of possible minor disturbances or interactions, as suggested by the slightly irregular shape and faint structures in the surrounding halo.
