The galaxy presents as a roughly elliptical structure with a high degree of central concentration. Its light profile appears smooth and lacking in distinct features such as spiral arms or a prominent disk. The core exhibits a yellowish hue, suggesting a population of older stars and relatively low levels of ongoing star formation. This central region transitions to a redder color that fades out around the edges of the galaxy, which may indicate a change in stellar populations. The overall shape suggests a system that has undergone significant dynamical relaxation. There is no indication of significant tidal disturbances or morphological abnormalities.