The galaxy exhibits an overall elliptical morphology. The central region is highly luminous, appearing nearly uniform in color, suggesting a significant concentration of older stellar populations. The luminosity decreases towards the outer regions, which appear somewhat elongated and less defined, possibly indicating a flattened spheroid shape. The overall color gradient transitions from a yellow-white core to a bluer hue in the outer regions, potentially indicative of ongoing, albeit possibly low-level, star formation in the galaxy's disk or outskirts. There is no clear evidence of spiral arms, bars, or significant dust lanes from the imagery. The morphology appears relatively undisturbed, with no obvious signs of a major ongoing merger event, although there may be evidence of minor tidal disturbance. Based on the elongation, the galaxy is not perfectly spherical, tending more towards a prolate shape.