The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated luminosity profile. It appears largely elliptical in shape, deviating only slightly from perfect circularity. The galaxy displays a color gradient, transitioning from a yellowish hue at the core to a subtly bluer periphery. There's no discernible spiral arm structure or prominent dust lane visible, suggesting a lack of significant ongoing star formation throughout the galaxy, but possibly more star formation occurring towards the outer regions of the galaxy. No strong evidence of any major mergers is observed, with the majority of the galaxy's light smoothly distributed. Slight signs of minor disturbances cannot be ruled out. Overall, it appears as a relatively evolved galaxy with a mass comparable to that of the Milky Way.
