The galaxy presents as a moderately bright object exhibiting a primarily smooth morphology. There is evidence of disk-like features, possibly in the form of faint spiral arms or a flattened structure. The central bulge appears distinct and relatively concentrated, with a slightly reddish hue. Surrounding the bulge, there are bluish regions indicating the presence of younger stellar populations and ongoing star formation. 

The overall shape is somewhat elliptical, with a ratio of major to minor axis greater than one. The galaxy shows signs of a potential interaction, or merger, with a small secondary galaxy, which is observed as a bright spot near the parent galaxy. This may be the cause of the disturbed disk morphology, indicating potential gravitational interactions. The colors indicate that this is most likely a spiral galaxy with intermediate levels of star formation.
