The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core, indicative of a significant stellar density. A diffuse halo surrounds the core, extending outwards with a gradual decrease in luminosity. The color profile suggests the presence of older stellar populations, with a dominant yellowish-orange hue, although faint hints of bluer regions are present in the outer edges, potentially indicating areas of recent, albeit limited, star formation. While the overall structure appears relatively undisturbed, there's a subtle asymmetry in the halo's extent, possibly hinting at minor tidal interactions or internal dynamic processes. There is no prominent disk, but a faint, patchy distribution of light suggests some irregularities within the galaxy's structure. 
