The galaxy presents as an elliptical-like structure with a smooth, concentrated central region. It appears predominantly yellow-orange in color, suggesting an older stellar population and a lack of significant ongoing star formation. There are faint extensions around this central region, which could be a sign of a disrupted system, possibly due to minor gravitational interactions. However, there is no clear evidence of a major ongoing merger. The galaxy appears to be in between being rounded and elliptical.
