The galaxy exhibits a disk-like structure, although its orientation is not precisely edge-on. Faint spiral arm features appear embedded within the structure. A central bulge is present, comprising a noticeable fraction of the galaxy's total luminosity. The galaxy's light is generally concentrated towards the center. There is evidence of a possible tidal tail like structure to the south west of the main body of the galaxy. There are no signs of a strong, well-defined bar structure bisecting the central bulge and disk. There is no intense star formation in the tidal feature. The galaxy's color suggests a mix of stellar populations, with a significant presence of older stars. Based on the observed morphology, the galaxy could be classified as a spiral or lenticular galaxy, with some features suggesting ongoing or recent interaction with another galaxy.
