This galaxy appears to be an elliptical galaxy, as it shows a generally smooth and rounded morphology. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy presents a yellowish-orange hue, suggesting a population dominated by older stars and a lower rate of recent star formation, or significant dust obscuration. There might be some minor disturbance in the galaxy shape that could be the result of an ongoing or past merger with another galaxy. The galaxy is quite compact.
