The galaxy presents an elongated morphology, exhibiting a distinct color gradient. The core region is characterized by a smooth, concentrated light profile with a yellowish-white hue, suggesting an older stellar population. Extending from this central region is a less defined, bluer component. This component appears less concentrated and possibly disk-like. There is a subtle asymmetry in the outer regions, potentially indicating a minor tidal disturbance or recent interaction. The overall structure suggests a galaxy transitioning from a more spheroidal, quiescent state to one with ongoing star formation within its disk-like regions.
