The galaxy presents a generally smooth, elliptical morphology, albeit slightly elongated in shape. The central region exhibits a brighter, more concentrated luminosity profile, indicative of a galactic nucleus. The light distribution fades gradually from the core outwards. There is subtle blotchiness present in the surrounding region that may be indicative of very minor irregularities within the galaxy's structure or dust obscuration. A slight color gradient is observed with bluer, more diffuse regions towards the edges, and warmer hues concentrated in the central part. The overall structure appears relatively undisturbed, showing no strong signs of ongoing major mergers or tidal interactions. 
