The galaxy presents as a relatively smooth, elliptical structure. Its overall form is predominantly round in appearance. The light distribution suggests a centrally concentrated luminosity profile. The color indices indicate a redder core region that shifts to bluer hues in the outer regions. There is a notable lack of distinct spiral arm features or prominent dust lanes, supporting the classification as an elliptical or lenticular galaxy. No prominent tidal tails or morphological distortions are readily apparent, however a possible minor disturbance is seen towards the bottom of the image. The galaxy appears to be relatively isolated.
