The galaxy presents a generally smooth appearance. Its overall form is elliptical, appearing round, with a high degree of central concentration. There is no indication of any spiral arm structure or significant dust lanes. The galaxy exhibits a radial color gradient, transitioning from a bright, almost white core, to yellowish hues in the outer regions. There appear to be no signs of major disturbances, mergers, or tidal tails, with only a subtle hint of possible minor disturbance. The overall color suggests an older stellar population, potentially indicating a low rate of ongoing star formation. 
