The galaxy presents a largely smooth, elliptical morphology. Its core exhibits a high degree of luminosity, suggesting a significant concentration of stars towards the galactic center. The galaxy appears relatively round, with only a slight deviation from perfect circularity. There is no apparent evidence of ongoing major mergers or significant tidal disturbances. The color gradient suggests a population of older stars, potentially indicating a low star formation rate. The faintness of any visible spiral arm structures reinforces a classification towards an elliptical or lenticular morphology.
