The galaxy exhibits an elongated, irregular morphology. Its structure appears to be disturbed, possibly indicating gravitational interaction or a recent merger event. The color profile suggests a dominant population of older stars, exhibiting reddish hues. There is a slight hint of bluer regions, potentially indicating pockets of star formation, although they appear subdued. Overall, the galaxy presents as a faint, relatively small object, suggesting either a significant distance or an intrinsic lack of luminosity. No clear spiral arms or a distinct central bulge are discernible, lending support to its classification as an irregular galaxy. The galaxy's shape deviates significantly from elliptical symmetry, implying a dynamic or disturbed state.
