The galaxy presents as a significantly elongated structure, appearing cigar-shaped in its overall morphology. Its central region is bright and relatively smooth, exhibiting a concentrated luminosity. A faint disk or a more complex structure is subtly visible, though indistinct.

There is no obvious evidence of a major ongoing merger, but a minor disturbance or possible tidal feature extending from the main body cannot be entirely ruled out. A slight distortion is noted in the main body. The galaxy demonstrates a relatively high degree of smoothness.

The dominant light emission appears to be in the green band, with weaker emissions in the red.
