The galaxy appears to be a relatively smooth, elliptical system. Its core is characterized by a bright, concentrated central bulge with a yellowish hue, suggesting an older stellar population. Moving outwards from the core, the galaxy displays a gradual decrease in surface brightness. A subtle disk feature may be present, but it is not sharply defined. The overall color gradient indicates a potential mix of stellar populations, with the core dominated by older, redder stars and the outer regions possibly containing a small fraction of younger, bluer stars. There appears to be no significant ongoing major merging events, though minor asymmetries or disturbances may be present, suggesting possible past interactions. The galaxy exhibits a generally round morphology, although some slight elongation or distortion is visible. Overall, the galaxy appears to be a mature, massive system.
