The galaxy presents as a relatively compact, elliptical object, with a smooth, diffuse light profile and a low surface brightness extending outwards. The central region exhibits a higher concentration of luminosity, suggesting a bulge component. There is no visual evidence of spiral arms or a prominent disk structure. The galaxy appears to be moderately red in color, indicative of an older stellar population and/or significant dust extinction. The isophotes are elongated and appear to be tilted along a northeast-southwest axis. There is no visual evidence of active galactic nuclei activity, or recent interactions.
