The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish hue, suggesting a population of older stars. A slightly less intense, greenish halo surrounds the core, possibly indicating the presence of ionized gas or a younger stellar population. The overall shape is somewhat rounded. There is no obvious evidence of spiral arm structure or major tidal disturbances, pointing towards a relaxed system. The colors suggest ongoing, though not extremely vigorous, star formation activity within the galaxy. The galaxy appears relatively isolated, with no apparent signs of interaction with nearby galaxies.
