The galaxy appears to be an elliptical galaxy with a smooth, somewhat round morphology. There is evidence of a possible merger or interaction event occurring. A secondary, smaller component is visible, slightly offset from the main body of the galaxy. There is a hint of a tidal tail or disturbed structure in the galaxy. The galaxy exhibits a generally red color, indicative of an older stellar population and lower star formation activity. The effective radius of the galaxy is approximately 4.5 kpc. The estimated stellar mass is relatively high, corresponding to a massive galaxy. The estimated star formation rate is moderately low, and the specific star formation rate implies a quiescent state.
