The galaxy appears to be a relatively small, but not dwarf-sized, system at an approximate distance corresponding to a redshift of z ~ 0.039. Its morphology is primarily smooth, although subtle features hinting at a disk structure are visible. The galaxy’s shape deviates from a perfect circle, tending toward an in-between roundedness. There's an indication of tidal disturbance or a past minor merger event evidenced by subtle asymmetries in the light distribution. The central region exhibits a relatively lower star formation rate. The object's spectrum indicates a mass around 10^8 solar masses. The magnitudes suggest this is a relatively dim galaxy in absolute terms. The galaxy presents a dominant smooth component, but the presence of disk-like features and signs of disturbance make it an interesting system for further morphological analysis.
