The galaxy appears to be an elliptical galaxy with a smooth, largely featureless morphology. It exhibits a concentrated, bright central bulge that gradually fades into the outer regions. The galaxy appears to have a slight elongation in its shape, transitioning from a circular form. There is no clear evidence of spiral arms or a distinct disk structure, suggesting it is likely a spheroidal system. The light distribution indicates an older stellar population, with the dominance of redder wavelengths. No significant tidal features or merging signatures are observed, indicating a relatively undisturbed evolutionary history.
