The galaxy presents as a likely interacting system exhibiting morphological disturbances. The primary component appears to be a moderately sized, edge-on disk galaxy with a central bulge. The bulge displays a yellowish-orange color, suggesting an older stellar population. The disk shows a bluer hue, potentially indicating ongoing star formation. 

A secondary component is visibly interacting with the disk galaxy. This companion exhibits a brighter, more irregular morphology. It has a knotty appearance and a brighter overall luminosity. There is a clear tidal bridge of material extending from the companion towards the disk galaxy, confirming the interaction. The galaxy's color suggests a slightly younger stellar population.

The combined system displays an elongated structure, approximately 6 kpc in radius. There is evidence of ongoing star formation within both galaxies. 
