The galaxy presents as a relatively small, faint spiral galaxy. The spiral arms are not well-defined and appear somewhat flocculent, lacking a grand design structure. The overall color suggests a moderate amount of star formation. The nucleus is not distinctly bright, indicating it may not have an active galactic nucleus. There is some visual evidence of minor disturbances or asymmetries in the morphology, possibly due to interactions, although no clear merging companion is apparent. The galaxy is largely composed of older stars, based on the redder hue throughout the disk, with regions of enhanced star formation. Overall, the galaxy does not seem to be going through a major interaction with other objects, even though its disk shape is not regular.
