The galaxy presents as a single, largely featureless object. It exhibits a smooth, elliptical morphology with a high degree of roundness. There is no apparent disk structure, spiral arms, or strong dust lanes visible. The color gradient suggests a central concentration of older stellar populations. The galaxy appears to be in an undisturbed state, with no obvious signs of recent or ongoing major merger activity, although some minor disturbances are not ruled out, especially in the upper part of the galaxy where the "body" is more circular and well defined, and the lower part is elongated. The redder color suggests low levels of on-going star formation.
