This galaxy exhibits a predominantly smooth morphology, with a high concentration of light toward the center, suggesting a significant bulge component. The overall shape appears close to round, with a slight deviation indicating it is somewhere in between a perfect circle and a more elliptical form. There are hints of faint, extended structure surrounding the central bulge, possibly representing a diffuse halo or disk. The color profile indicates a generally older stellar population with a reddish-yellow central region, surrounded by more blueish colors. This color gradient may imply ongoing, albeit relatively low-level, star formation in the outer regions. There are only subtle indications of disturbances, such as asymmetries in the light distribution, possibly signifying past minor merger events. Overall, the galaxy presents as a relatively evolved system, transitioning, or having already transitioned, towards a quiescent state.
