The galaxy presents a morphology consistent with an elliptical type, appearing largely smooth and featureless. Its overall shape is slightly elongated, deviating minimally from perfect circularity. The galaxy exhibits a concentrated central bulge that decreases in intensity outwards from the center. Its color appears to be on the redder side, suggesting a population of older stars. There are no apparent signs of ongoing major mergers or significant tidal disturbances affecting the overall structure of the galaxy, although a very minor interaction cannot be ruled out.
