The galaxy presents as a disk galaxy, viewed at an intermediate inclination. The central bulge appears significant, with a high surface brightness and a yellowish hue, possibly indicating an older stellar population. A flattened disk surrounds the bulge, exhibiting a bluer color, indicative of ongoing star formation. The disk shows hints of spiral structure, though it is somewhat diffuse and lacks well-defined arms. There may be some disturbances within the structure of the galaxy.
