The galaxy presents a largely smooth, elliptical morphology. The central bulge is prominent, displaying a concentrated luminosity with a yellowish hue, indicative of an older stellar population. Moving outwards from the core, the galaxy exhibits a gradual decrease in surface brightness. A faint, diffuse halo surrounds the central region, characterized by a bluer color, possibly suggestive of more recent star formation in the outer regions. While the overall structure appears largely undisturbed, a slight asymmetry is visible in the outer edges of the halo, potentially hinting at minor gravitational interactions or past merger events.
