The galaxy presents as a singular, relatively smooth structure. It appears elliptical in shape, with a dominant central bulge. The galaxy exhibits a concentrated distribution of light, with a high degree of central luminosity that decreases gradually towards the outer edges. No distinct spiral arms or bar features are readily apparent. The color profile is generally yellow, indicating an older stellar population, with a possibility of low ongoing star formation. There is no evidence of a major merger, but a minor disturbance cannot be ruled out.
