The galaxy presents as a moderately bright, relatively smooth object with a somewhat elongated, cigar-like morphology. The central region exhibits a pronounced, bright core, suggesting a high concentration of stars or possibly an active galactic nucleus. A faint disk component is visible, although not sharply defined, exhibiting a slight color gradient from the central bulge outwards. There is a subtle bluing of the disk indicative of possible recent star formation. No major disturbances or clear signs of ongoing mergers are evident. The overall appearance suggests a disk galaxy viewed at a significant inclination, with a dominant bulge.
