The galaxy presents a generally smooth morphology, suggesting it is likely an elliptical galaxy. The galaxy exhibits an overall golden hue, possibly indicating a population of older stars. A slight elongation is visible in the image, but the galaxy is mostly round. No signs of spiral arms, dust lanes, or any major disturbances can be seen. It appears to be a fairly isolated galaxy, showing no signs of interaction with other galaxies. There is likely a high amount of ongoing star formation. The estimated diameter of the galaxy is around 10 kiloparsecs.
