The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. There is no clearly defined spiral structure visible. The galaxy's light profile seems relatively uniform, with a concentrated central region that gradually fades outward. Color variations are subtle, trending towards redder hues across the galaxy's body. Overall, the galaxy gives the impression of a mature system with an older stellar population and a low ongoing star formation rate. Light suggests it is a massive galaxy. There may be a minor merging event occurring. 