The galaxy presents an overall elongated, cigar-shaped morphology. It exhibits a smooth light distribution, lacking prominent spiral arms or significant patchy features. The core of the galaxy appears brighter and more concentrated, with a yellowish hue, indicating a possible older stellar population. The color becomes slightly redder as it moves toward the outer edges of the galaxy. There is no apparent dust lane visible. Evidence suggests it is not undergoing a major merger. However, it also does not appear perfectly round which may indicate a past merger.
