This galaxy exhibits a primarily smooth morphology, with a color gradient transitioning from a yellowish core to a redder outer region. The overall shape is elliptical, appearing slightly elongated rather than perfectly circular. There is no obvious spiral arm structure or significant dust lane obscuration visible in this image. The light distribution appears concentrated towards the center, suggesting a higher stellar density in the core. There is minimal evidence of major disturbances or ongoing merger activity, although subtle asymmetries could indicate a minor interaction in its past. The redder color in the outer regions may suggest an older stellar population and reduced star formation activity. The overall appearance is consistent with an early-type galaxy.
