This galaxy presents as a generally smooth, elliptical structure. There is a distinct central bulge exhibiting a yellowish hue, suggesting an older stellar population concentrated at the core. The surrounding halo appears less defined, with a bluer tint indicating the presence of younger stars and possibly some ongoing star formation, albeit at a relatively low rate. There is no clear evidence of a prominent disk or spiral arms; instead, light smoothly decreases in intensity from the center to the outer regions. The galaxy exhibits a high degree of circularity with no significant morphological disturbances, hinting at a gravitationally relaxed system, possibly with no recent major merger events. There is a slight elongation, but overall the galaxy appears relatively round. Given the observed color gradients and morphology, this system seems to be a mature galaxy with a stellar mass toward the higher end, suggesting a slow but persistent rate of star formation.
