The galaxy exhibits a generally smooth morphology, suggestive of an elliptical or lenticular classification. Its overall shape appears relatively round. A concentrated central bulge is present, surrounded by a more diffuse halo. There is a slight hint of a faint disk-like structure extending from the bulge, however, a definitive classification is difficult given image resolution and the lack of prominent spiral arms or distinct features. Faint blueish regions are present and concentrated in one region of the disk, possibly indicating localized star formation. Overall, the object has a significant mass, and a relatively low rate of star formation for its size. Possible merger or tidal effects are present.
