The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal with a noticeable concentration of light towards the center. The core exhibits a brighter, yellowish hue, suggesting a higher density of older stars. The outer regions display a gradual decrease in luminosity and a transition to a slightly bluer color profile, implying the presence of younger stellar populations, though these are less prominent than the core's older population. The galaxy shows a slight elongation, deviating marginally from a perfectly circular shape; however, there are no obvious signs of spiral arms, a prominent disk structure, or major tidal disturbances suggestive of ongoing or recent major merger events. The overall structure indicates that the galaxy is relatively evolved and stable, potentially experiencing a low rate of current star formation.
