The galaxy presents an elliptical morphology, though some irregularity is observed. The core of the galaxy exhibits a high surface brightness, appearing smooth and concentrated. A gradient of decreasing luminosity extends outward from the core. The surrounding galactic envelope demonstrates a more diffuse nature, with hints of asymmetrical structure. Faint, irregular features are present in the outer regions, possibly indicating minor disturbances or tidal interactions. The color profile shows a shift toward redder hues in the central bulge, suggesting an older stellar population. In contrast, the outer regions appear slightly bluer, potentially indicating ongoing or recent star formation activity.
