The galaxy appears to be an elliptical type, characterized by a smooth, relatively featureless morphology. There is a dominant central bulge, exhibiting a yellowish hue, suggestive of an older stellar population. The overall shape is close to circular. There seems to be some disturbance in its gravitational structure, potentially signs of a recent or ongoing merger event as indicated by the asymmetric shape and minor tidal distortions. Evidence exists of redder regions, possibly implying areas with more dust or older star clusters.
