The galaxy presents a predominantly cigar-shaped morphology, appearing elongated along its major axis. There is a central bulge region with a concentrated luminosity gradient, exhibiting a smooth, diffuse appearance. The color of the bulge is slightly redder in comparison to the outer regions of the galaxy. Fainter, bluer extensions are visible along the major axis. The outer regions of the galaxy appear less defined, lacking distinct spiral arm structures. There is no clear evidence of active galactic nuclei or significant dust lanes. The overall structure suggests an evolved system, possibly undergoing a transition from a spiral to an elliptical morphology. No signs of tidal disruption or ongoing major mergers are readily apparent, but there are some minor disturbances that can be observed.
