The galaxy presents a diffuse, somewhat irregular morphology. It displays a faint, bluish hue, suggesting the presence of recent or ongoing star formation. No distinct spiral arm structures are readily apparent. The overall shape is somewhat elongated, with a central region appearing slightly brighter and more concentrated. There's a suggestion of some disruption to the galaxy's structure, potentially indicative of tidal interactions or a minor merger event. No prominent bar structure is visible within the central region. The light distribution does not appear to be dominated by a large, prominent bulge, but rather a more uniform, disk-like structure.
