The galaxy appears as a single, largely homogenous object with a smooth, elliptical morphology. Its light profile is concentrated towards the center, with a general decrease in luminosity with radial distance. The core of the galaxy exhibits a yellowish hue, suggesting an older stellar population or a significant dust presence. The outer regions show a slight blue tinge, potentially indicating more recent star formation activity, though this is subtle. No distinct spiral arms or bar structures are visible, and there are no obvious signs of tidal disturbances or ongoing major mergers. The overall structure suggests a well-mixed stellar population with a relatively quiescent evolutionary history.
