The galaxy presents a generally smooth appearance with a slight elongation, suggesting a shape somewhere between elliptical and lenticular. The light distribution is centrally concentrated, fading gradually towards the edges with no discernable spiral arms. The color appears relatively uniform across the galaxy, with a hint of blue light, suggesting the presence of some young stellar populations, though not dominating the overall color. There is no strong evidence of recent major merger activity or significant tidal disturbances in the immediate vicinity, though a subtle asymmetry may indicate past interaction. The central region appears brighter and slightly more compact than the surrounding halo. The overall impression is that of a mature galaxy with an intermediate mass, potentially undergoing low levels of star formation.
