The galaxy appears as a slightly elongated structure, suggesting a possible elliptical morphology, or a disk galaxy viewed at an angle. The central region exhibits a bright, concentrated luminosity, indicative of a dense stellar population or an active galactic nucleus. There is some disturbance in the morphology of the galaxy, with faint plumes extending outwards. Some degree of rotational symmetry is present, but there are subtle asymmetries. Color gradients are visible, transitioning from a yellowish core to bluer outer regions.
