The galaxy appears as an elliptical or lenticular type, exhibiting a generally smooth light distribution. The central region of the galaxy presents a concentrated luminosity, suggesting a significant stellar population. There is very little indication of spiral arm structure, star formation regions, or dust lanes, suggesting that this galaxy is a relatively passive system, either an elliptical or a quiescent spiral. The galaxy presents as a yellowish color, with little in the way of blue light, supporting the idea that it has older stars, and little current star formation. There is no obvious evidence of tidal interactions, merging, or major disturbances within the galaxy's morphology. The light profile suggests a centrally concentrated shape with a smooth, continuous decline in brightness outward from the core.
