The galaxy presents a somewhat amorphous, diffuse morphology. It appears relatively smooth in structure, lacking prominent spiral arms or a well-defined central bulge. The color profile indicates a dominant population of older stars, with a noticeable lack of strong blue emission that would suggest active, ongoing star formation. A slight elongation is observed, although the overall shape is generally rounded. There is a suggestion of minor disturbances in the galaxy's structure, potentially indicative of past interactions or mergers. Overall, this galaxy appears to be an evolved system that may have undergone significant morphological transformation through various processes, potentially in a quiescent state with minimal current star formation.
