The galaxy appears to be a relatively smooth, early-type system. The light distribution is centrally concentrated, showing a gradual decline in intensity outwards from the core. There is little evidence of spiral arms or a prominent disk structure. The galaxy exhibits an elliptical morphology, appearing moderately round with some elongation. There is no visually obvious ongoing major merger activity, although subtle irregularities might indicate minor disturbances or past interactions. The system displays a general lack of blue color, suggesting an older stellar population and a low ongoing star formation rate. The overall color profile is dominated by redder wavelengths. The galaxy is likely a massive system.
