The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, with a slight extension suggesting a disk component. The color gradient indicates potential radial variations in stellar populations, with a bluer hue towards the outer edges, hinting at possible ongoing star formation activity there. Faint indications of minor tidal disturbances may be present, suggesting possible past interactions. Overall, the galaxy appears to be a moderately massive system, with a mix of evolved and younger stellar populations.
