The galaxy appears to be a relatively luminous, early-type system. Its morphology is predominantly smooth, with a significant fraction of the citizen science votes identifying it as such. The shape is noticeably elongated, leaning toward a cigar shape, suggesting it is an elliptical galaxy viewed at an angle. There may be a slight suggestion of a faint, diffuse disk, but this is difficult to discern.

The galaxy's color gradient indicates a redder central region, suggesting an older stellar population with ongoing star formation. There is no pronounced evidence of spiral arms or significant dust lanes. Based on the redshift, this galaxy is at a considerable distance. There seems to be evidence of disturbance in the system.
