The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge with a radial decrease in luminosity outwards. The color is generally yellowish-white, indicative of an older stellar population, although there may be some slight color variation. There is no easily observable spiral structure or prominent dust lanes. The galaxy's shape is mostly round but exhibits slight disturbances suggestive of a past or ongoing minor merger event. There is no strong evidence of current, significant star formation based on the image's color composition.
