The galaxy appears as a diffuse, faint, bluish object. The morphology is somewhat irregular, lacking a clearly defined nucleus or spiral arm structure. There is a slight elongation, but its overall structure is amorphous, it does not appear to be a standard elliptical or spiral type. 

There is evidence of disturbance within the galaxy's structure. Some regions appear slightly brighter and denser than others, suggesting possible ongoing star formation or tidal interactions. The color gradients across the galaxy are subtle but noticeable, with a shift towards bluer hues in certain areas, again indicative of star-forming regions. There is also a faint patch off to one side which could be tidal arm or the remnant of a smaller galaxy being disturbed. 

Overall, the galaxy presents as a disturbed system potentially undergoing a minor merger event. Additional spectral data would be useful to confirm the age and composition of the stellar populations present.
