The galaxy appears to be an elliptical or lenticular galaxy exhibiting a smooth, centrally concentrated bulge. The galaxy has a somewhat elongated shape. There is no strong evidence of spiral arms or a well-defined disk. The color gradient indicates the presence of an older stellar population, with a redder central region, and the hint of a bluer region towards one of the ends, suggesting a small amount of recent star formation. There is no clear indication of tidal features or significant morphological disturbances, indicating that it may not be undergoing a major merger.
