The galaxy presents as a diffuse object with an irregular morphology. At first glance, it does not display a well-defined spiral or elliptical structure.

The galaxy exhibits a mottled appearance, suggesting localized regions of differing stellar populations or dust obscuration. There are hints of disturbed features, with some faint extensions or tidal tails indicating potential past or ongoing interactions. Patches of bluer color are visible, particularly clustered towards the lower-left, suggesting active star formation regions. The central region appears less concentrated, without a distinct bulge, but rather a nebulous distribution of stars and gas. Overall, the galaxy's light is spread relatively evenly across its observable extent.
