The galaxy presents a somewhat amorphous morphology. The central region is characterized by a bright, concentrated core that appears yellowish. Surrounding the core is a broader, less defined disk or halo-like structure, exhibiting a bluer hue. The light distribution within this outer region appears relatively smooth, with minimal evidence of distinct spiral arms or prominent dust lanes. The overall form suggests a galaxy undergoing some form of interaction or disturbance, potentially a minor merger event. There seems to be a faint hint of tidal features or extended diffuse emission, though this is not definitive. The observed colors suggest ongoing, though possibly subdued, star formation.
