The galaxy presents as an elliptical morphology, appearing largely smooth and featureless in this observation. It exhibits a concentrated central bulge, with a gradual decrease in luminosity moving outwards, suggesting a relatively even distribution of stars within the spheroid. The galaxy displays a dominant yellowish-orange hue, indicative of an older stellar population with lower levels of recent star formation. There is a hint of bluer light in the outer edges of the object, potentially indicating a small amount of recent star formation. Based on the observed morphology, there is no evidence of major mergers or significant tidal disturbances. It appears round in shape with no features suggesting any significant recent interactions. 
