The galaxy appears as a faint, diffuse object. It is slightly elongated, with a shape that is more in-between elliptical and disk-like. The light distribution seems relatively smooth and centrally concentrated, with no distinct spiral arm structures or a prominent central bulge immediately apparent. There is a suggestion of some minor disturbances or asymmetries in the light distribution, possibly indicating interactions or minor mergers, but the galaxy's overall structure does not appear to be heavily disrupted. Color gradients across the galaxy are subtle, but suggest bluer components in the inner regions, possibly due to on-going star formation. The galaxy is relatively compact.
