The galaxy presents a mostly smooth morphology, with a significant fraction of its light distributed in a spheroidal component. There is some evidence of a disk-like structure, though it is not sharply defined. The overall shape is neither perfectly spherical nor highly elongated.

There are potential signs of minor disturbances in the galaxy's structure, possibly indicating a past or ongoing interaction. These disturbances do not appear to be major mergers, however.

The galaxy exhibits a relatively blue color in the optical bands, which could be related to ongoing star formation. Based on the red shift it can be determined this galaxy is not extremely distant. 
