The galaxy presents as a single, moderately bright object with a centrally concentrated morphology. The light profile appears relatively smooth, with no distinct spiral arm structures or prominent dust lanes visible. The color appears broadly yellow-white, indicating a possible mix of stellar populations, with some contribution from older, redder stars. A slight asymmetry in the light distribution could suggest a minor interaction or disturbance event. The galaxy's apparent roundness suggests that it may be either a face-on spiral or potentially an elliptical galaxy. The absence of clearly defined features implies a system where the light is dominated by an older stellar population, or is seen at a great distance.
