The galaxy presents as a relatively smooth, elliptical-like structure. Its color is generally yellow, suggesting an older stellar population. The central region appears more concentrated and brighter, potentially indicating a bulge. The isophotes are somewhat elongated, with a slight deviation from perfect circularity. There is a subtle indication of a possible minor disturbance or interaction visible in the outer regions, without clear evidence of a major ongoing merger event. Star formation appears low, consistent with the galaxy's dominant color.
