The galaxy exhibits a generally smooth morphology with a hint of a disk-like structure. Its shape is elongated, appearing somewhat cigar-shaped rather than perfectly round. A distinct color gradient is observed across the galaxy, shifting from bluer hues on one side to redder tones on the other, potentially indicating differential stellar populations or dust obscuration. There is faint evidence of a possible minor disturbance in the galaxy's structure, perhaps due to a past or ongoing interaction. The overall light distribution suggests a relatively low star formation rate. The galaxy's mass appears to be within the range of a dwarf galaxy.
