The galaxy presents a somewhat diffuse and indistinct morphology. There is evidence suggesting it may exhibit characteristics of both an elliptical and a spiral galaxy; specifically, the lack of defined spiral arms could indicate a more spheroidal form, yet some faint disk-like structures and possible arms are visible. Color gradients suggest a radial variation in stellar populations and/or dust content. The central region appears brighter and possibly more yellow/red, which may be due to an older stellar population. The outer regions appear slightly bluer, which may be due to a younger stellar population, but the details are not resolvable in this image. There are subtle indications of tidal disturbances or asymmetries, with the outer edges slightly irregular, possibly indicative of past interactions or minor mergers. Further investigation with higher resolution imaging and spectroscopic data would be necessary to determine the exact nature of this galaxy.
