The galaxy presents an overall elliptical morphology, appearing largely smooth with a concentrated central bulge. The light distribution suggests a gradual decrease in brightness from the core outwards. A slight elongation is visible, indicating it is not perfectly spherical. The color profile shows a central region that appears yellowish-white, transitioning to a more reddish hue in the outer regions of the galaxy, possibly indicating an aging stellar population in the outskirts. There are subtle indications of tidal disturbances, potentially suggesting an interaction or past merger event. Further analysis would be required to confirm these features.
