This galaxy exhibits an elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures. There is a notable concentration of light towards the galactic center, indicating a bright central bulge. The light distribution suggests a relatively high degree of radial symmetry.

Subtle color gradients are discernible. The central region appears more yellowish-orange, possibly indicating an older stellar population. Progressing outwards, the color shifts slightly towards a blueish-green hue, which could suggest the presence of younger stars, although not to a significant extent. 

There is no evidence of ongoing major mergers or strong tidal disturbances within the visible data. Minor disturbances cannot be ruled out completely. The galaxy appears somewhat elongated, but not drastically so. It appears to be an isolated system.
