The galaxy presents as a relatively small, disk-shaped structure with a notably faint and diffuse appearance. It exhibits a somewhat irregular morphology, lacking a well-defined spiral arm structure. The light distribution appears clumpy, suggesting ongoing or recent star formation activity across the galactic disk. Patches of blue light indicate regions of hotter, younger stars, while the overall redder hue of the disk implies an older stellar population and/or the presence of dust obscuring some regions. There may be some evidence of minor gravitational disturbances or interactions, as indicated by slight asymmetries in the disk. The central region doesn't show a pronounced bulge, indicating a disk-dominated morphology. Overall, this galaxy appears to be a relatively quiescent system with a subdued rate of star formation.
