The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. It exhibits a nearly spherical morphology, displaying little deviation from a circular form. There is a faint, diffuse halo surrounding the central region, gradually fading into the background sky. The galaxy shows a redder color profile, suggesting a population of older stars and a relatively low rate of ongoing star formation. There is no evidence of a prominent disk structure or spiral arms. No signs of any major merger events or tidal disturbances are evident. The overall appearance indicates a relatively evolved, quiescent galaxy.
