The galaxy presents as an elliptical morphology, with a somewhat elongated shape. The light distribution appears smooth and centrally concentrated, suggesting an older stellar population. There is a subtle color gradient visible, with a slightly bluer hue in one region which could indicate some recent star formation activity, though the overall color is indicative of evolved stars. No prominent spiral arms or dust lanes are discernible. There is a faint hint of disturbance or tidal feature, though subtle and challenging to characterize with precision. The galaxy appears relatively isolated, without any obvious signs of a major ongoing merger event.
