The galaxy presents an overall elongated, cigar-shaped morphology. The central region exhibits a bright, yellowish hue, suggesting a concentrated population of older stars. Fainter bluish extensions are observed emanating from both ends of this central bulge, possibly indicating areas of more recent star formation within a disk-like structure. There is a subtle hint of asymmetry in the distribution of the bluer regions, but no obvious signs of major tidal disturbances or ongoing mergers are apparent. The galaxy's structure appears relatively smooth, although some subtle irregularities in the faint outer regions cannot be ruled out. The galaxy is relatively distant.
