The galaxy presents as a single, relatively smooth object with a concentrated central bulge. There is a slightly elongated shape to its overall form, appearing somewhat cigar-shaped rather than perfectly spherical. The light distribution is dominated by a yellowish hue, suggesting a stellar population with a relatively low rate of ongoing star formation. The lack of clearly defined spiral arms or dust lanes indicates that it may be an elliptical galaxy or a lenticular galaxy with a large bulge. There is a hint of some fuzziness along the edges, but overall the object appears well resolved. There may be some evidence of past interactions, but nothing is disrupting the overall shape of the galaxy. 
