The galaxy exhibits a central bulge that appears yellowish-white, suggesting an older stellar population. Extending outward, a fainter, bluer disk is observed, indicative of more recent star formation activity. The disk is not perfectly symmetrical, showing some subtle irregularities. There is no strong evidence of a spiral structure. Based on its color profile, the galaxy is likely undergoing moderate levels of star formation. The object presents as a system that may be classified as an intermediate stage between a spiral and an elliptical galaxy. There are also some indications of minor disturbances.
