The galaxy presents as a relatively smooth, elliptical or lenticular structure with a central bulge and an extended halo. The overall color appears yellowish-orange, suggesting a population of older stars with relatively little ongoing star formation. Its morphology is generally round, with a subtle deviation from perfect circularity. No distinct spiral arms or bar structures are visible. There seems to be a slight asymmetry in the halo, hinting at a possible minor interaction or disturbance. The light distribution indicates a concentration of older stars toward the center, with decreasing stellar density further out in the halo. There is no clear evidence of a major ongoing merger.
