The galaxy presents as a single, relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing largely spheroidal in shape, with a moderate degree of roundness. The galaxy's core is luminous, suggesting a concentration of older stars. The galaxy shows no prominent spiral arm structures or significant dust lanes. There is a lack of obvious tidal features or disturbances, indicative of a relatively quiescent state, possibly the result of a previous minor merger event. The light profile appears to fade gradually from the central core outwards. There is no strong evidence of ongoing star formation, suggesting this is an older system.
