The observed galaxy presents as an elliptical-like system with a concentrated, luminous core. The galaxy's overall morphology appears relatively smooth, with a high degree of central concentration. There are no obvious spiral arms or significant dust lanes visible in this imagery. The color profile transitions from a yellowish-white core to a bluer periphery. There may be slight indications of a mild disturbance or interaction with a satellite galaxy, evident in the faint, diffuse extensions.
