The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. There is a slight elongation observable, though the overall shape approximates a spheroid. The core of the galaxy appears bright and yellowish, indicating an older stellar population. There is a color gradient moving outward, with a faint bluish tinge toward the outer edges. This suggests the presence of some younger, bluer stars within the galactic disk, though star formation rates are likely low overall. There is no clear evidence of spiral arms or prominent dust lanes; the morphology is largely featureless. There is no clear evidence of mergers or tidal disturbances in the vicinity, so the galaxy appears relatively isolated.
