The galaxy presents an irregular morphology, exhibiting a structure that deviates significantly from a well-defined spiral or elliptical form. The overall color is yellowish-orange, suggesting an older stellar population with a diminished presence of young, hot, blue stars. There are a few regions with redder hues, possibly indicating areas of dust obscuration or older stellar populations. The light distribution is clumpy and uneven, suggesting that the galaxy may be undergoing some form of gravitational interaction or internal disruption. It has a faint, diffuse appearance with no obvious nucleus, leading to the possibility of it being a low-surface-brightness dwarf galaxy or a system undergoing a merger. Furthermore, there is no evidence of spiral arms or a prominent disk. The structure of the galaxy is amorphous, perhaps indicating a late-stage merger with other galaxies.
