The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology. The galaxy displays a single, distinct nucleus. There are no discernible spiral arms or a prominent disk structure. The color distribution across the galaxy is varied, with a higher concentration of redder hues towards the center, possibly indicating an older stellar population. The galaxy shows signs of potentially ongoing or recent merger activity, presenting an irregular shape and some light distortion in the overall structure. Despite the potential merger, the bulk of the galaxy has a fairly round appearance. The estimated size indicates that the galaxy is a moderately large galaxy. Based on its colors, stellar mass and estimated star formation rate, the galaxy seems to be in the process of aging or quiescence.
