The galaxy presents a largely elliptical morphology, exhibiting a high degree of central concentration. The light profile appears smooth with a strong radial gradient, transitioning from a very bright, nearly unresolved core to a more diffuse outer halo. The overall color is consistent with an older stellar population, suggestive of relatively little current star formation. There is a very slight hint of a disk with a few small pockets of star formation visible. The galaxy appears isolated with no obvious signs of tidal disturbance or interaction with other galaxies.
