The galaxy presents a generally smooth, elliptical morphology, displaying a high degree of central concentration. The light profile appears relatively undisturbed, lacking significant tidal features or strong asymmetries suggestive of recent major merger activity. The galaxy exhibits an elongated shape, although the axis ratio indicates it is not highly flattened. The primary color is a yellow-ish white, suggesting that the galaxy is mostly comprised of older stars. There is no prominent indication of dust lanes or spiral arm structures. A very minor disturbance may be present in one section of the galaxy, although the evidence is limited. The projected size appears relatively small.
