The galaxy presents as a slightly elongated, disk-like structure. A central bulge is visible, appearing relatively bright and concentrated. The overall color is bluish, with the central region displaying a more yellow/white hue, possibly indicating an older stellar population in the bulge. Faint spiral arm structures are possibly present, although not sharply defined. Some irregular features are also observed within the galactic disk, suggesting possible minor disturbances, perhaps due to interactions. The galaxy seems relatively isolated with no obvious major companions or signs of ongoing major merger activity, although minor tidal features can't be ruled out.