The galaxy appears as a centrally concentrated object with a largely smooth, elliptical morphology. There is a distinct lack of spiral arm structure. The galaxy exhibits a radial color gradient, appearing more yellow or reddish toward the core, suggesting an older stellar population. There is a slight color change towards the outer edges of the galaxy, becoming slightly more blue, but very slight.

The smooth appearance and radial color gradient suggest minimal ongoing star formation within the galaxy at this time. There is no evidence of any major disturbances, such as tidal tails or obvious signs of an ongoing or recent merger event. The galaxy appears relatively isolated.
