The galaxy appears as a centrally concentrated elliptical or lenticular system. Its overall shape is elongated, with a cigar-like morphology. There is a smooth light distribution, suggesting a well-mixed stellar population. There is little evidence of spiral arms or significant dust lanes. The central region is brighter, with a gradual decrease in luminosity outward. The galaxy appears to be isolated. Based on its color and morphology, the galaxy likely hosts a relatively low rate of star formation. 
