This galaxy appears as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. The core region exhibits a higher surface brightness, gradually decreasing outwards towards its fainter edges. There is a slight blueish hue to the central region, which may indicate ongoing star formation, although the smooth texture suggests it is not a strongly star-forming galaxy. There appears to be little evidence of well-defined spiral arms or prominent dust lanes, implying it is likely not a classic spiral galaxy. Faint irregularities or disturbances may be present in the outer halo of the galaxy which suggests minor gravitational interactions. The overall shape is fairly round.
