The galaxy presents as a relatively compact and luminous object. It exhibits a smooth, elliptical morphology, appearing largely spheroidal in shape with minimal discernible disk structure. The central region is bright and concentrated, suggesting a significant stellar population density. A slight elongation is observed along one axis, but overall, the galaxy approximates a circular form. A subtle color gradient exists, transitioning from a yellowish hue at the core to slightly bluer tones in the outer regions, potentially indicating varying stellar populations and ages. While the general appearance is smooth, there may be subtle signs of minor disturbances in the outer regions or a faint tidal feature, but without more detailed imagery it is hard to say for sure. There may be a hint of on-going or recent mergers. Overall, the object appears to be a moderately massive system with signs of possible evolutionary processes at work.
