The galaxy appears to be a relatively smooth, elliptical type, exhibiting a centrally concentrated light profile. The shape is neither perfectly spherical nor significantly elongated, appearing somewhere in between. The overall color is yellowish-orange, suggesting a population of older stars and a lower rate of ongoing star formation. There is no visual evidence of spiral arms or a prominent disk structure. No major merging events appear to be taking place, as the galaxy seems relatively undisturbed. There is very subtle, minor disturbance visible to the upper left.
