The galaxy presents as a centrally concentrated object with a moderate degree of smoothness. The morphology suggests a possible elliptical galaxy or perhaps a lenticular galaxy with a dominant bulge, seen nearly edge-on. There is a subtle hint of some disturbance or asymmetry in the outer regions but this is not consistent. It is also possible that this is the result of noise in the imaging data. The central region appears more luminous than the extended halo. Overall, the galaxy appears relatively quiescent in terms of star formation activity. There are no bright, young stellar populations discernible in the available image, indicating the presence of older stars. There is a subtle color gradient. The central bulge appears relatively redder compared to the fainter outer regions.
