The galaxy presents a largely smooth, elliptical morphology. It appears as a centrally concentrated object with a radial decrease in surface brightness. The core exhibits a bright, unresolved nucleus indicative of concentrated stellar population, potentially a supermassive black hole. The galaxy's overall color suggests an evolved stellar population, possibly dominated by older, redder stars, but there is indication of bluer light as well. There are no obvious signs of spiral arms or significant dust lanes. The overall structure seems largely undisturbed, with no apparent major merging events or strong tidal features visible within this observation. The galaxy appears well-defined with a regular, generally spheroidal shape, with an apparent size consistent with a moderate-sized galaxy.
