The galaxy presents as a smooth, centrally concentrated object, exhibiting an elliptical morphology. It displays a bright, yellowish core indicative of an older stellar population. The isophotes appear generally smooth, with a slight elongation along its major axis, suggesting it is not perfectly spherical. There may be a faint blue halo surrounding the central region, possibly indicative of a small amount of recent star formation in the outer regions. No spiral arm structures or significant dust lanes are discernible within the image resolution. Subtle disturbances appear present, but these are classified as minor. The galaxy may be undergoing a minor merger, but is most likely undisturbed.
