The galaxy appears to be an interacting system, likely composed of two distinct galaxies in the process of merging.

One galaxy presents as a highly inclined disk galaxy, possibly even edge-on. This galaxy exhibits a noticeable dust lane along its major axis, obscuring the light from the galactic bulge. The overall color is relatively red, suggesting an older stellar population. 

The second galaxy is more diffuse and appears spheroidal or elliptical. It is noticeably bluer in color, implying a younger, more actively star-forming stellar population. The shape of this galaxy is less defined, possibly due to tidal disruption caused by the interaction with the disk galaxy.

There is evidence of tidal features, such as faint extensions of light extending outward, suggestive of gravitational interactions. The system exhibits a complex morphology, likely a result of the ongoing merger event.
