The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards the outer regions. There is a slight elongation, but overall, the galaxy appears quite round. The galaxy has a dominant yellowish hue in its central regions, which suggests an older stellar population. Some faint blue tinges appear around the core. No obvious signs of spiral arms, dust lanes, or active star formation regions are visible. The morphology suggests a passively evolving system with little current star formation, which aligns with the redder colors observed. There appears to be a very slight disturbance in the lower right quadrant which may indicate a minor tidal interaction.
