This galaxy exhibits a primarily smooth morphology, suggesting an elliptical or lenticular classification. The central bulge appears prominent, with a high degree of symmetry. There is a hint of a disk-like structure, though it is not sharply defined. No significant spiral arm structure is discernible. The galaxy appears slightly elongated rather than perfectly spherical. There is no obvious evidence of on-going major merging events, though some minor disturbances might be present. Its color suggests a population of older stars with limited active star formation. Overall, it appears to be a relatively massive galaxy.
