The galaxy presents as a spiral type, displaying distinct, loosely wound spiral arms. A significant portion of the light is concentrated in what appears to be a central bulge. The color gradients suggest differing stellar populations, with the central regions exhibiting a yellow/orange hue, potentially indicative of older, redder stars, while the spiral arms show hints of bluer tones, suggesting younger, hotter stars and ongoing star formation. One dominant spiral arm can be distinguished, while other arms appear to blend together. No strong bar feature is immediately apparent, however, there is a hint of an offset within the central bulge that could imply a weak bar presence. The structure of the galaxy is quite disturbed, it appears to be undergoing a merger or recent tidal interaction which contributes to the disturbed morphology.
