The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be primarily elliptical, exhibiting a somewhat intermediate shape between perfectly round and elongated, with a slight preference towards the latter. There is no discernible spiral arm structure. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal distortions. There is a suggestion of minor disturbance. The color profile indicates a redder overall population, indicative of an older stellar population with potentially lower ongoing star formation. The effective radius of the galaxy appears compact. The galaxy appears at a distance where individual star-forming regions or dust lanes cannot be resolved.
