The galaxy presents as a primarily smooth structure, exhibiting a slightly elongated, cigar-shaped morphology. The central region displays a high concentration of light, suggesting a prominent galactic bulge. The light distribution gradually diminishes outwards from the center, forming a diffuse halo. There is a subtle hint of a flattened structure suggestive of a disk, but no distinct spiral arms or bars are visible. The overall color appears somewhat red, which could indicate an older stellar population with low recent star formation activity. There is no obvious evidence of significant tidal disturbances or ongoing mergers.
