The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. The central region displays a yellowish-orange hue, likely indicative of an older stellar population. The galaxy lacks any discernible spiral arm structures or prominent dust lanes. There may be some hints of subtle, extended outer regions, displaying a faint bluish tinge. The overall structure suggests a fairly evolved system, likely an elliptical or lenticular galaxy, showing no indications of significant recent merging events or major disturbances.
