This galaxy presents a generally smooth morphology, with minimal apparent internal structure. The light distribution appears somewhat centrally concentrated, exhibiting a gradual falloff in surface brightness from the center outwards. There is a subtle elongation or asymmetry visible, potentially indicating a slight tidal disturbance or past interaction. Color gradients across the galaxy appear subtle. The galaxy's overall color seems consistent with an older stellar population, but higher resolution imagery or spectroscopic data would be required to confirm this. There is also no obvious dust lane and no obvious signs of merging activity.
