The galaxy presents as a largely smooth, elliptical-like structure, appearing moderately compact with a concentrated central bulge. The core region exhibits a yellowish-orange hue, suggesting an older stellar population dominated by evolved stars. Moving outward from the core, a gradual color shift towards a bluer, less defined halo is observed, potentially indicating the presence of younger stars, although star formation appears subdued. The overall shape is not perfectly spherical; a slight elongation is noticeable along one axis. There are hints of minor disturbances in the outer regions but the galaxy presents no clear evidence of ongoing major mergers. Its morphological profile is predominantly smooth, with only a small fraction showing the presence of distinct disk-like features.
