The galaxy presents a complex, possibly interacting morphology. A dominant, relatively amorphous central region exhibits a smooth appearance with a concentration of light towards the core. This area is ellipsoidal in shape, with a length scale of an estimated 4.7 kpc. Evidence of a tidal tail or disrupted arm extends from this central region, suggesting a potential interaction or past merger event.

The colors observed indicate a mix of stellar populations. The core of the central region appears to be a bluer hue, which would indicate relatively new stars. The faint tidal arm has a yellower hue which indicates relatively old stars. 

Overall, the galaxy shows characteristics consistent with an ongoing or recent interaction, with the central region representing a merging core and the extended feature signifying the remnants of a tidal interaction. Star formation appears to be suppressed.
