The galaxy presents a morphology that appears to be somewhat disturbed. There is no clear spiral arm structure or a well-defined disk. The light is relatively diffuse, with a slightly brighter central region. The overall shape is elongated, but not extremely so. The galaxy exhibits a hint of blue coloration, which could indicate ongoing star formation, although not at a very high rate. There is some asymmetry in the distribution of light, which could be due to minor tidal interactions or internal disturbances. There may also be an indication of a faint tidal tail or bridge extending away from one side of the galaxy, though it is hard to clearly tell.
