The galaxy exhibits an elliptical morphology with a high degree of central concentration of light. The core region presents a bright, compact, and somewhat indistinct nucleus. Moving outward from the core, the galaxy gradually fades in intensity. The overall color profile suggests a higher concentration of older stellar populations, as indicated by the reddish hue observed in the outer regions of the galaxy, while the central region may have younger, hotter stars. There's an absence of prominent spiral arm structures or significant dust lanes. The general smoothness indicates a galaxy that may be relatively evolved and undisturbed.
