The galaxy presents as a relatively smooth, lenticular-like structure with an intermediate ellipticity. The light distribution suggests a dominant bulge component. There appears to be a subtle disk-like structure with faint and disturbed features. No prominent spiral arms are discernible. There may be a slight disturbance that could be a minor merger event. The galaxy exhibits a redder color, indicating an older stellar population and potentially lower ongoing star formation. Overall, the galaxy appears as a evolved system transitioning towards quiescence.
