The galaxy presents a slightly elongated, ellipsoidal morphology. A central bulge is visible, exhibiting a yellowish-orange hue, possibly indicative of an older stellar population and/or dust obscuration. The outer regions are less defined, appearing more diffuse with a subtle blue-green tint. There is some suggestion of spiral arm structure but is subtle and may also be merging features. The overall structure shows evidence of disturbance, possibly due to a recent or ongoing merger event.
