The observed galaxy presents as a faint, elongated structure. There is evidence of a disk-like morphology, although the central bulge is not particularly prominent. One arm of the galaxy appears more extended. The color profile of the galaxy suggests a possible mixture of stellar populations, with bluer regions indicating ongoing star formation, especially at the extended arm. There is a subtle asymmetry in the galaxy's overall shape, possibly indicating minor gravitational disturbance or tidal interactions. The galaxy exhibits a slight diffuse halo extending beyond its main structure.
