The galaxy presents a somewhat disturbed morphology, suggesting possible interactions or recent mergers. The core region appears relatively smooth and concentrated, exhibiting a yellowish hue, indicative of an older stellar population. Moving outwards from the core, there is evidence of a more extended disk-like structure with bluer patches scattered throughout. This colour variation likely corresponds to pockets of more recent star formation. The overall structure appears asymmetric, with some irregularities in the outer regions suggesting tidal features or disrupted arms. There is no singular, clear spiral structure, suggesting that this could be a more amorphous galaxy, possibly in transition, between spiral and elliptical.
