The galaxy presents a relatively smooth and concentrated morphology. It exhibits a yellowish central region, suggesting the presence of an older stellar population. There may be some evidence of a very weak and diffuse disk, although it is difficult to confirm due to its smooth appearance. Any spiral arms or bar structures are indistinct. The galaxy is approximately round in shape, with a fairly high mass, and a low specific star formation rate, all suggesting a galaxy with a relatively passive stellar population. There does not appear to be any obvious major tidal disturbance or ongoing merger activity.
