The galaxy presents as a relatively large, well-defined disk galaxy oriented nearly edge-on to our line of sight. It exhibits a prominent central bulge, appearing smoothly rounded and concentrated in luminosity. The disk is visible as a flattened structure extending outward from the bulge. There are no obvious signs of major mergers, but the disk could have some minor distortions. The galaxy appears generally smooth in texture, and no distinct spiral arm features or prominent dust lanes are discernible, though the edge-on perspective would obscure these. The color distribution suggests that the bulge is likely dominated by older stellar populations, while the outer regions might contain a mix of stellar ages.
