The galaxy appears as a centrally concentrated object with a smooth light distribution. It is roughly elliptical in shape, exhibiting a moderate degree of roundness. There is evidence of a possible merger event, indicating that the galaxy may be interacting with another galaxy in the background or foreground, or that it has undergone a merger in the past. The galaxy displays a redder color, suggesting an older stellar population and a potentially lower rate of on-going star formation. The size of the galaxy appears moderate, not excessively large or compact.
