The galaxy presents a largely smooth, elliptical morphology. A slight elongation is visible, but it is predominantly rounded in appearance. There is a subtle color gradient, with a central concentration of yellowish-orange hues, suggesting a population of older stars. Fainter bluish tones are also present, perhaps indicating pockets of more recent star formation. There is no distinct spiral arm structure or significant dust lane obscuration visible. It does not appear to be undergoing any major merging events or displaying strong tidal disturbances based on its morphology.
