The galaxy appears to be an elliptical type, with a smooth, concentrated light profile. There is a distinct, bright central bulge. Moving outwards from the center, the light intensity decreases gradually. There is a slight elongation, giving the appearance of being somewhat flattened, but not resembling a spiral disk. The galaxy presents a yellow-orange color, which suggests a population dominated by older stars. There are no obvious spiral arms or dust lanes visible. The overall structure implies a relatively quiescent galaxy with little ongoing star formation. There is no evidence of any major ongoing merger events, though the galaxy appears slightly distorted.
