This galaxy presents as a slightly disturbed spiral galaxy with a prominent central bulge. There is evidence of ongoing star formation, particularly within the arms of the galaxy. The overall color is a mix of older stellar populations within the central bulge, exhibiting a redder hue, and younger, bluer stars distributed throughout the spiral arms.

Dust lanes are subtly visible within the arms, obscuring some of the starlight. The disk of the galaxy is slightly inclined relative to our line of sight. The spiral arms appear somewhat flocculent, rather than well-defined. There are potential signs of minor tidal disturbances, suggesting possible past interactions with another galaxy. The estimated size, around 6.7 kpc, suggests a smaller to average spiral galaxy for its type.
