The galaxy appears to be an elliptical galaxy, or at least a lenticular type, as it exhibits a smooth, relatively featureless morphology with a high degree of central concentration. It presents an elongated, cigar-like shape. The light distribution suggests a lack of prominent spiral arms or a well-defined disk. The galaxy's color index seems to indicate a population of older stars, and minimal active star formation. There is no apparent sign of any ongoing or recent major merging activity or significant tidal disturbances; it appears to be a relatively isolated system. 
