The galaxy presents an elongated morphology with a prominent central bulge. There is evidence of a disk structure, with visible arm-like features extending from the central region. The distribution of light suggests a non-uniform stellar population, with bluer regions possibly indicating areas of active star formation, particularly at the Eastern end of the galaxy. Redder hues are concentrated in the central bulge and to the western end of the galactic disk. There is a visible disturbance in the main structure that appears to be caused by an ongoing or recent merger. This is supported by the overall irregular shape. The galaxy presents signs of tidal distortions in its disk structure. The size of the galaxy is approximately 6 arcseconds across.
