The galaxy presents as a single, resolved object with no apparent spiral arm structure. Its form leans towards a flattened ellipsoid, nearly round, but not perfectly so. The galaxy exhibits a multi-colored hue, suggestive of diverse stellar populations. There are areas that appear a darker red, while others are a brighter yellow. The galaxy’s light profile suggests it is likely a quite massive system undergoing a merger event. The shape of the merger appears that it will coalesce into a system dominated by older stellar populations with a relatively low star formation rate. The overall structure is somewhat disturbed, indicating possible past interactions or ongoing accretion events.
