The object appears to be a galaxy exhibiting characteristics of a disturbed system. There is an indication of tidal tails and asymmetrical features suggesting a potential ongoing or recent merger event. The main body of the galaxy presents a diffuse appearance, lacking a well-defined nucleus, which may be due to active star formation or a disrupted morphology. There is an indication of a blueish tint on the upper edge of the galaxy, possibly due to younger stars. It also has some redder regions, likely to be due to older stars. The overall structure is irregular, deviating significantly from a typical elliptical or spiral form.
