The galaxy presents as a relatively smooth, elliptical object with a high degree of roundness. It exhibits a centrally concentrated light profile, suggesting a dominant bulge component. There is no apparent spiral structure. Faint colour variations within the galaxy may indicate subtle differences in stellar populations. Overall, the galaxy appears undisturbed, with no obvious signs of tidal features or ongoing major mergers, although the presence of a smaller companion galaxy nearby could indicate some interaction. The galaxy shows strong signs of being quite old, with faint signs of recent star formation. 
