The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or early-type spiral. The light distribution is fairly uniform, lacking prominent spiral arm structures or distinct features typically associated with active star formation regions. The galaxy exhibits a near-circular morphology, showing only slight deviations from perfect roundness. The galaxy has a moderate redshift, indicating it is not among the closest galaxies. There is no indication of any major ongoing merger activity or significant tidal disturbances affecting the galaxy's overall structure, although minor disturbances cannot be ruled out. The object appears to have a relatively low star formation rate, contributing to its redder color.
