The galaxy appears to be an elliptical type. It exhibits a smooth, relatively featureless morphology, with a somewhat elongated shape. The central region is brighter and more concentrated, gradually decreasing in luminosity towards the outer edges. The color profile suggests a population of older stars, with a yellowish hue dominating the galaxy's appearance. There is no readily apparent evidence of spiral arms or significant dust lanes. The overall structure suggests a system that is well evolved, with a spheroidal distribution of stars. There are no visible signs of any major disturbances.
