This galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is elliptical in nature, with a slight elongation that suggests a transition from a perfectly spherical shape. A dominant, bright central bulge is apparent, characterized by a yellowish hue, possibly indicating an older stellar population. The outer regions exhibit a gradual decrease in luminosity, with hints of bluer tones, suggesting the presence of younger stars or ongoing star formation at a lower rate than observed in more active spiral galaxies. No significant disturbances or tidal features are visually detected, indicating a relatively undisturbed evolutionary history. The galaxy appears to be undergoing little to no major merger activity based on its overall regular structure. The size appears moderate.
