The galaxy presents as a relatively smooth, elliptical or lenticular structure. The color is predominantly yellow to red, suggesting an older stellar population with a lower rate of star formation. It exhibits a centrally concentrated brightness profile that fades gradually towards its outer regions. The overall morphology indicates a high degree of symmetry and a lack of prominent spiral arms or significant dust lanes. There may be a smaller galaxy nearby exhibiting a blueish tint, but it is difficult to tell if the two are interacting. The galaxy exhibits a slightly elongated shape, but is mostly circular. No merger is currently occurring.