The galaxy appears to be a relatively smooth, elliptical or lenticular system. Its light is concentrated towards the center, with a gradual decrease in intensity outwards, suggesting an evolved stellar population. The object exhibits a generally round morphology, with no significant deviations indicating a strong departure from axial symmetry. There is a hint of a central structure, possibly a small disk feature viewed at an oblique angle or a central bar. There may be signs of interaction with other galaxies. Overall, this galaxy has a smooth, fairly undisturbed structure.
