The galaxy presents as a generally smooth and elliptical object. Its overall shape approximates a rounded form, exhibiting minimal features indicative of a prominent disk structure or ongoing major merger activity. There is some indication of minor disturbance of the surrounding stars around the object. The central region displays a higher concentration of luminosity, with a gradual decrease in brightness towards the outer edges. Color gradients suggest a dominant population of older stars. It is likely a massive galaxy with very little star formation. The galaxy may be located a great distance from our own.
