The galaxy presents as a relatively smooth, concentrated object. Its overall shape is approximately round, with some slight deviation from perfect circularity. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the center, the color subtly shifts to a redder tone, implying a change in stellar population and potentially the presence of dust. There is no apparent spiral structure or distinct features such as bars or rings. The lack of obvious morphological disturbances suggests it is not currently undergoing a major merger event. Faint, diffuse light extends outwards from the central region, but the overall light profile is centrally concentrated. The galaxy appears to be a relatively quiescent system with little active star formation.
