The galaxy presents a somewhat elongated morphology. There is a hint of a disk-like structure, though it is not sharply defined. The central region appears brighter and more concentrated, possibly indicating a central bulge. A subtle colour gradient is observed across the galaxy, with the central regions showing a more yellow hue, potentially suggesting an older stellar population, while the outer regions exhibit bluer tones, indicative of more recent star formation activity. There is no clear evidence of significant tidal disturbances or major mergers, but a slight asymmetry might suggest minor interaction or internal processes shaping its structure. The overall appearance suggests a galaxy in a relatively quiescent state, with ongoing but not extreme star formation.
