The galaxy appears to be an elliptical or lenticular type. It has a generally smooth morphology with no discernible spiral arms or bar structure. The light distribution suggests a centrally concentrated bulge, fading gradually towards the outer regions. It appears to be somewhat spheroidal in shape, with a high degree of roundness, with no cigar shape. There are no obvious signs of a major merger or significant tidal disturbances, but there may be indications of minor disturbances in the outer regions. The color suggests a relatively older stellar population, consistent with a low star formation rate.
