The galaxy presents as a moderately luminous object, exhibiting a generally smooth morphology. The light distribution suggests a centrally concentrated structure, with a slight elongation, deviating somewhat from a perfectly circular form. There is a subtle color gradient across the galaxy; the central region appears more yellow and the outer regions appear more blue, possibly indicating a relatively quiescent stellar population in the core and more active star formation in the outer areas. There's no visible evidence of strong spiral arm structures, major disturbances, or ongoing merger activity. However, subtle irregularities in the light distribution might suggest minor interactions or internal dynamical processes. Overall, the galaxy appears relatively evolved, likely with a substantial stellar mass.
