The galaxy presents as an elongated, disk-like structure, seen at an oblique angle. The central bulge appears moderately bright and concentrated, exhibiting a smooth texture. The disk component shows a slight blueish hue and is not fully resolved, appearing relatively smooth with indistinct spiral arm structure. The galaxy's overall color suggests ongoing, but not exceptionally high, rates of star formation. The shape indicates a possible classification as a spiral galaxy viewed at an angle, or potentially a lenticular galaxy. There is no obvious sign of tidal disturbances or major merging events, but minor perturbations cannot be ruled out at this resolution. The galaxy's relatively small size suggests a dwarf galaxy.
