This galaxy presents as a relatively smooth, centrally concentrated object. The core exhibits a bright, yellowish-white hue, suggesting a significant population of older stars. There is a slight radial color gradient, with the outer regions appearing somewhat bluer than the central bulge, hinting at the presence of younger stars in the outer disk. The galaxy's overall shape approximates an elliptical or lenticular morphology, showing no obvious spiral arm structure or signs of a major ongoing merger. There might be a very slight distortion in its shape, which could indicate a minor interaction or disturbance.
