The galaxy presents as a somewhat elliptical structure, not a perfect circle. Its overall color profile suggests a mix of stellar populations, with a bright, concentrated core exhibiting a more yellowish-white hue, possibly indicating a higher density of older stars. Fainter, bluish regions appear to extend from the central core, hinting at ongoing or recent star formation. The galaxy shows signs of a disk-like structure, viewed at a relatively small angle. Overall, the galaxy does not seem to show signs of significant interaction or disturbance.
