The galaxy presents a largely smooth and elliptical morphology. It appears as a single, concentrated light source with a noticeable radial gradient in brightness. The central region exhibits a yellowish hue, suggesting a population of older stars. There is a subtle extension of light outwards from the core, indicating a gradual decrease in stellar density with increasing radius. Some subtle, faint wisps or features are barely visible, which could indicate minor tidal disturbances, though these are not prominent. The overall shape is somewhat elongated, tending towards an elliptical form. There is no clear evidence of spiral arms or a distinct disk component.
