This galaxy presents as a lenticular or possibly a spiral galaxy seen at a high inclination, nearly edge-on from our line of sight. The main body of the galaxy exhibits a smooth, centralized luminosity that gently fades away from the center. The central bulge appears moderately defined, with an elongated shape consistent with the edge-on view. 

There is some evidence for a faint, extended disk component, though it is relatively subtle and compact. It may possess a faint spiral structure, but its presence cannot be definitively confirmed due to its small size and the image's limitations. The galaxy lacks clear indications of ongoing, intense star formation regions, which would manifest as bright, blue knots in the disk.

Overall, the galaxy's morphology suggests it is a relatively evolved system with a dominant bulge and a less prominent disk, exhibiting low current star formation activity. No obvious signs of a major merger event are apparent, although minor disturbances in the disk's structure might be present.
