The galaxy presents as an edge-on spiral, exhibiting a flattened disk morphology. The bulge appears smooth and concentrated, with a spheroidal shape. The dust lane, although not sharply defined, is implied from the light attenuation along the midplane of the disk. The galaxy shows no signs of major tidal disturbances or significant morphological asymmetry, suggesting it has not experienced a recent major merger. The visible color profile suggests an older stellar population. The star formation rate appears to be low. The galaxy's mass is relatively high, indicating that it's a fairly massive galaxy.