The galaxy appears as a moderately bright, yellowish-white object. Its shape is generally smooth, with a somewhat elliptical form, tending toward round rather than cigar-shaped. There is no obvious evidence of a disk component. The galaxy appears centrally concentrated, lacking distinct spiral arms or a clear bar structure. No significant tidal features or signs of ongoing major merging events are immediately apparent, however, there might be subtle signs of minor disturbance in the faint outskirts of the galaxy. The color suggests a relatively older stellar population, with lower rates of star formation. The object is reasonably compact.