The galaxy appears as a relatively compact object. Its morphology suggests a smooth, elliptical shape with a high degree of roundness. There is no visible evidence of spiral arms or a prominent disk structure. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions.

The galaxy exhibits a color gradient, appearing somewhat bluer in its central regions. There is no indication of significant ongoing mergers or major disturbances affecting its overall structure. The galaxy is approximately 3.9 kiloparsecs in radius and has a substantial stellar mass. However, it also seems to have low specific star formation.
