The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. The core region exhibits a strong yellowish-white color, suggestive of an older stellar population. The isophotes appear moderately elliptical, transitioning towards a more diffuse, bluer periphery. There's a slight asymmetry in the outer regions, with a subtle extension visible on one side. No prominent spiral arms or distinct dust lanes are discernible within the image resolution. There is no evidence of a major merger event, although minor disturbances can not be ruled out at this resolution. The galaxy appears to be intermediate in roundness, not perfectly spherical nor highly elongated.
