The galaxy presents as a spiral galaxy with a redshift of approximately 0.1369. It exhibits a notable disk structure, viewed at a slight angle to our line of sight, indicating it is not precisely edge-on. The presence of spiral arms is evident.

The bulge of the galaxy appears moderately sized, with a bright central concentration of light, indicating the possible presence of an active galactic nucleus.

There is no obvious sign of major disturbances or ongoing mergers within the galaxy. The light distribution appears relatively smooth in the disk. 

The galaxy is brighter in redder bands than bluer bands, indicating older stellar populations as expected with the absence of major mergers.

