The galaxy presents with a somewhat amorphous morphology. The core region exhibits a relatively smooth, high-intensity profile. This central region shows a distinct green hue, possibly indicating a concentration of ionized oxygen or other emission line activity. The galaxy extends outwards from this core, with the intensity gradually decreasing. The outer regions show a more diffuse and irregular structure, with faint wisps or extensions visible primarily on one side. The overall color of the outer regions shifts towards a bluer shade, possibly indicating the presence of younger stellar populations or a contribution from scattered light. There is a subtle asymmetry to the galaxy's overall shape, which could be indicative of a past or ongoing interaction with another galaxy, though no other distinct galaxy is immediately apparent in this image. Further spectroscopic analysis would be needed to determine the galaxy's redshift, star formation rate, and the composition of its interstellar medium.
