The galaxy appears to be an elliptical galaxy, characterized by its smooth and featureless morphology. It presents a nearly perfect circular profile, with minimal deviation from roundness. The light is concentrated towards the center, exhibiting a bright, well-defined core that gradually decreases in intensity with increasing radius. There is no evidence of spiral arms, bars, or other distinct structural components commonly found in disk galaxies. No signs of mergers or tidal disturbances are visible, which would manifest as asymmetries or irregular shapes. The galaxy exhibits a color profile consistent with an older stellar population. The galaxy appears to be a relatively massive and quiescent system with low star formation.
