The galaxy exhibits a prominent spiral structure, characterized by two well-defined spiral arms that extend outwards from a central bulge. These arms appear to be loosely wound. The central bulge of the galaxy exhibits a moderate size, and a relatively smooth, condensed appearance. A possible bar structure appears to be present. Evidence of merging or tidal interaction with a companion galaxy is present. The object's apparent color suggests a mix of stellar populations, from younger blue stars to older, redder stars within its structure. The red shift indicates it is an extra-galactic object.
