The galaxy presents a largely smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish hue. The light distribution transitions smoothly from the core outwards, with the outer regions appearing more diffuse and slightly bluer in color, suggesting the potential presence of a population of younger, bluer stars at larger radii. There is little evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or tidal interactions, though a possible minor disturbance cannot be ruled out. The round appearance suggests a minimal inclination relative to our line of sight. Overall, this galaxy appears to be a massive and relatively evolved system with moderate star formation activity.
