The galaxy presents as a relatively small, faint object. Its overall morphology appears disturbed, possibly indicating an ongoing or recent interaction. The central region exhibits a brighter, more concentrated luminosity. There is an asymmetry in the galaxy's light distribution, hinting at tidal features or uneven star formation. No distinct spiral arms or bar structures are clearly discernible. The color profile suggests a mix of stellar populations, with some regions appearing bluer and others redder, possibly indicating a range of ages and metallicities within the galaxy. There might be a slight elongation or distortion in the shape.
