The galaxy appears to be a single, relatively smooth object, exhibiting a concentrated central region with a gradual decrease in luminosity towards the outer edges. The overall shape is elliptical with a high degree of roundness, showing no pronounced disk-like structures or spiral arms. The color gradient suggests an aging stellar population, with the central bulge exhibiting a yellow-orange hue. There is no obvious sign of significant ongoing star formation within the galaxy, as indicated by the lack of bright blue regions. The morphology of the galaxy is fairly uniform, showing no major signs of tidal disturbances or interaction with other galaxies, although a slight asymmetry could indicate a minor interaction in its past.
