The galaxy presents as a moderately luminous, early-type system, likely an elliptical or lenticular galaxy, based on its smooth, featureless morphology. There is no discernible disk or spiral structure. The light profile suggests a high degree of central concentration, with the brightest region located at the galaxy's core. The color appears relatively uniform, with a yellow-orange hue, suggestive of an older stellar population dominated by red giant and red dwarf stars. The absence of blue light indicates minimal on-going star formation. The isophotes appear generally round, showing minimal evidence of tidal disturbances or recent merger events. The size of the galaxy appears to be relatively compact.
