The galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, exhibiting a bright, well-defined core. Moving outward from the core, the light intensity gradually decreases, lacking any distinct spiral arm structures or prominent features, like bars or rings, that would indicate a disk component. There are no obvious signs of recent or ongoing major mergers, and the galaxy seems relatively undisturbed. The colour appears slightly blueish, especially towards the outer regions, suggesting at least some ongoing star formation. It has a roughly circular shape.