The galaxy presents a primarily smooth morphology, with a high degree of central concentration. Its overall shape appears elliptical or lenticular, with a notable lack of spiral arm structure. There is some deviation from perfect circularity, leaning towards an in-between roundness. No signs of ongoing major mergers or significant tidal disturbances are visually apparent. The galaxy exhibits a color profile suggesting a population of older stars, with the red band appearing more intense than the blue band. This could indicate that star formation rates are relatively low within the galaxy. 
