The galaxy presents a largely smooth and rounded morphology. Its central region exhibits a concentrated, bright yellowish-white glow, indicative of a significant population of older stars. There is a subtle, almost imperceptible, extension of light emanating from the core, suggesting a faint, diffuse halo. No spiral arm structures are discernible, which, combined with the smooth appearance and yellow-white color, implies an evolved stellar population and potentially reduced ongoing star formation activity. The galaxy appears relatively isolated, showing no obvious signs of recent or ongoing major merger activity, though minor disturbances cannot be ruled out.
