The galaxy presents a somewhat amorphous, diffuse morphology. A central, brighter region is apparent, suggesting a concentration of stars and possibly a central bulge. The surrounding structure exhibits a less defined, more irregular shape, possibly indicating the presence of a disk component. There are subtle color variations across the galaxy, with slightly bluer hues in the outer regions. These bluer colors suggest the presence of younger, hotter stars, possibly indicating ongoing or recent star formation in these areas. There's also evidence of possible disturbance in the structure.
