The galaxy presents a largely elliptical morphology, appearing quite smooth in structure with little evidence of spiral arms or a prominent disk. The light distribution is highly concentrated towards the center, indicating a bulge-dominated system. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The outer regions transition to a redder color. There are only minimal signs of tidal disturbances or ongoing merger activity. Overall, the galaxy appears to be a fairly relaxed and evolved system.
