The galaxy presents a largely smooth, elliptical morphology with minimal visible features. The central region exhibits a concentrated, yellowish hue, suggesting a population of older, redder stars. Moving outward from the core, a gradual transition occurs towards a more diffuse, bluish halo. This bluer component hints at the presence of younger, hotter stars and possibly some ongoing, though subdued, star formation. The overall shape appears somewhat oblate, falling between a perfectly round and cigar-like form. There is no clear evidence of spiral arms or a distinct disk structure. Minor disturbances or merging activity are not readily apparent in this image.
