The galaxy appears to be a spiral type, characterized by a central bulge surrounded by a relatively well-defined disk. Prominent spiral arms extend outwards from the central region. These arms exhibit a somewhat patchy structure, suggesting regions of active star formation. The winding of the spiral arms appears to be of an intermediate nature, neither tightly wound nor completely open.

The central bulge presents a yellowish hue, indicating a population of older stars. The spiral arms show a bluer coloration overall, suggestive of younger, hotter stars and ongoing star formation. There are also several areas of more intense red or orange color in the arms, which can indicate regions with a significant presence of dust or areas of older stellar populations within the arms. 

There appears to be some disturbance in the morphology of the galaxy. Further analysis of spectral data is required to determine whether the disturbance is caused by gravitational interaction with another galaxy, or some other event.
