The galaxy presents as a centrally concentrated object with a smooth overall morphology. There is an indication of a slight elongation, deviating marginally from a perfectly circular form, as well as a hint of a disk-like structure. The central region exhibits a yellowish-white hue, which likely signifies an older stellar population. The outer regions display a faint greenish-blue tint, possibly suggestive of ongoing, albeit low, star formation. There are no immediately apparent signs of significant tidal disturbances or major merging events. The galaxy appears relatively isolated and stable.
