The galaxy presents as a somewhat irregular, diffuse object. Its overall shape appears elongated, with a brighter, condensed central region and fainter, more extended edges. The light distribution suggests a disk-like structure, although it lacks a well-defined spiral arm pattern. The color is predominantly bluish-white, indicating the presence of a younger stellar population and active star formation. Patches of slightly redder hues are observed within the galaxy, potentially representing older stellar populations or dust lanes. There is evidence of some minor gravitational disturbance, with the possible presence of tidal features or asymmetries in the outer regions. No clear central bulge is visible. The galaxy's appearance suggests it is a relatively low-mass system, possibly a dwarf galaxy or a late-type spiral galaxy with a low star formation rate.
