The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. There's a high degree of rotational symmetry. The galaxy exhibits a color gradient, appearing bluer towards the central region and becoming redder in the outer regions. The overall color suggests an older stellar population. There are no obvious signs of spiral arms or ongoing major mergers, though some minor disturbances cannot be ruled out due to the image resolution. The galaxy is moderately elongated, with a major axis roughly twice the length of the minor axis.