The object appears to be a spiral galaxy with a relatively compact core and a prominent disk. The spiral arms are somewhat diffuse and do not exhibit a tightly wound structure. There is evidence of minor disturbances in the outer regions of the galaxy, which could be indicative of a previous interaction or ongoing minor merger event. The galaxy shows a mix of stellar populations, as indicated by the variations in color. Some regions are bluer, suggestive of younger stars and ongoing star formation. There are also redder regions, indicating the presence of older stellar populations. The overall morphology suggests that the galaxy is likely in a relatively late stage of its evolution, although the potential interaction could be triggering localized star formation. A notable feature is the overall "fuzziness" of the galaxy, which could be due to significant amounts of dust obscuring parts of it. The galaxy does not exhibit a classical grand design spiral structure.
