The observed galaxy presents a complex morphology. There appears to be a central, bright region, possibly indicative of a galactic nucleus. Extending outward from this core, faint disc-like structures are observed. The overall form is not smoothly elliptical, showing evidence of disturbances. There are possible features resembling spiral arm fragments, although the definition is poor. The color distribution is uneven, with areas of bluish emission and reddish emission. Some reddish structures are observed. There is no clear central bulge. The features suggest that the galaxy may have undergone recent interactions with a smaller galaxy or experienced disturbances.
