The observed galaxy presents a somewhat irregular morphology. It appears as a diffuse, patchy structure with no distinct nucleus or spiral arm features evident in the image. The overall color is bluish-white, suggesting the presence of younger stellar populations within the galaxy. There are regions of slightly enhanced blue emission, indicative of possible ongoing star formation. The galaxy does not exhibit a smooth, elliptical profile; instead, its light distribution is rather clumpy. There is also a clear, though faint, tidal stream or disrupted feature suggesting a past merger, or ongoing interaction with a smaller galaxy. A clear, but dim blue area in the center may suggest the presence of either a bright star cluster, or a bulge that is being obscured by dust. The galaxy seems to be surrounded by a faint halo.
