The galaxy presents as a centrally concentrated object with an apparent smooth morphology. The color profile indicates a greater concentration of redder wavelengths towards the core, suggesting an older stellar population in that region. The outer regions, while still smooth, exhibit a subtle shift towards bluer wavelengths, potentially indicating the presence of younger stars or regions of ongoing star formation, though at a relatively low rate. The galaxy appears to be generally elliptical, with a slight deviation from perfect circularity, showing it is slightly oblong. There is no obvious evidence of tidal tails, strong gravitational lensing, or ongoing major merger events. Faint, subtle asymmetries in the outer regions hint at a possible minor disturbance or past interaction.
