The galaxy presents an elliptical morphology, appearing relatively smooth and featureless. Its light distribution indicates a centrally concentrated bulge that gradually fades outwards. The primary color of the galaxy is a yellowish-orange hue, suggesting an older stellar population with a low rate of ongoing star formation. The overall shape is slightly elongated. There is no clear evidence of spiral arms or significant dust lanes. The galaxy appears to be relatively isolated with no obvious signs of interaction with neighboring galaxies, although very minor disturbances cannot be ruled out based on this image alone.
