The galaxy presents as a disk galaxy with a moderate inclination relative to our line of sight. A prominent central bulge, with a yellowish-white color, dominates the galaxy's core, indicating an older stellar population. The disk component displays a bluer hue, suggesting the presence of younger, hotter stars and ongoing star formation, especially on one side of the galaxy. There's a slight asymmetry and a suggestion of some disturbances, potentially indicating minor gravitational interactions or past merger events. The galaxy has a relatively smooth overall structure, and its shape appears somewhat elongated.
