The galaxy presents as an elliptical morphology, exhibiting a largely smooth and rounded appearance. The concentration of light is highly centralized, with a gradual decrease in surface brightness moving outward from the core. The color profile is dominated by yellowish hues, indicating an older stellar population. There is little evidence of spiral arms or significant dust lanes. The overall structure suggests a system that is dynamically relaxed, likely a result of past mergers or a cessation of active star formation. No clear signs of tidal disturbances or interactions with neighboring galaxies are visible.
