The galaxy presents as a luminous, relatively smooth object with a concentrated central bulge. The light is evenly distributed, and there is minimal evidence of distinct spiral arm structures or prominent dust lanes. The galaxy appears largely elliptical in shape. There is no indication of any major ongoing merger events or strong tidal disturbances, with only a hint of minor asymmetry or a possible faint arm. The color suggests a population of older stars and a low ongoing rate of star formation.
