The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology with a high degree of rotational symmetry. The central bulge region is bright and appears nearly spherical. The color profile suggests a somewhat evolved stellar population, with a subtle reddening observed in the outer regions compared to the bluer central core. This indicates either a radial gradient in stellar age and composition, or a differential dust extinction effect. There are no obvious spiral arm features, bar structures, or tidal tails visible, suggesting a relaxed morphology. Possible minor disturbances are inferred by the slight non-uniformity of the outermost regions. Overall, the galaxy likely resides somewhere on the continuum between elliptical and lenticular galaxies.
