The galaxy presents as a likely merger of two distinct components. The primary body appears elongated with a central concentration of light, indicative of a bulge or nucleus. Its overall color is relatively redder, suggesting an older stellar population. The secondary component is less defined, appearing more diffuse, and exhibits a bluer tint hinting at more recent star formation. A bridge of material seems to connect the two components, with a greenish hue that is likely attributed to ongoing star formation. Tidal features are subtle, suggesting either an early stage merger or a merger where interactions have largely dissipated the more dramatic tidal tails. The galaxy is mostly smooth in appearance but shows some features that could possibly be a disk.
