The galaxy exhibits a flattened, disk-like morphology, as suggested by its elliptical shape. The central region presents a bright, concentrated core, potentially indicative of an active galactic nucleus or a dense stellar population. Moving outwards from the core, a less defined, diffuse structure is observed. The surrounding disk appears somewhat disturbed or irregular, showing hints of possible tidal interactions or recent minor mergers. There's a redder region along one side, hinting that there could be a small tidal tail or dust lane. Overall, the galaxy's structure suggests that it may be actively evolving through interactions or internal processes, though a larger sample and deeper study are needed to confirm.
