The galaxy appears as a relatively small, faint, and elongated object. Its morphology is likely that of an edge-on spiral or lenticular galaxy, exhibiting a smooth, centralized bulge with a faint disk extending outwards. There is no clear evidence of spiral arm structure or prominent dust lanes. The galaxy's color seems to be generally blue-white, indicating a presence of relatively young, hot stars, albeit not overwhelmingly so. The overall shape and appearance do not suggest any significant interaction or recent merger events, but it may be difficult to completely rule out minor disturbances given the image quality. The galaxy appears to be quite distant.
