The galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated. There is little evidence of spiral arms or significant disk structure. The light distribution suggests an overall spheroidal shape with a gradual decline in brightness from the core outwards. 

The color profile is moderately red, indicating a population of older stars. There may be minimal ongoing star formation as indicated by the overall color and lack of strong blue emission indicative of hot, young stars. There seems to be a minor disturbance or possible tidal feature, but it is difficult to tell from the image. The galaxy seems to be fairly isolated. 
