The galaxy presents an elongated, elliptical morphology. A prominent central bulge is observed, exhibiting a concentrated luminosity gradient, suggesting a high stellar density. The overall color profile shifts from a warmer, yellower hue in the nucleus to slightly cooler, redder tones extending outwards along the major axis. While it's difficult to discern fine details, there is a suggestion of a faint, diffused disk component surrounding the bulge. No distinct spiral arm structures are immediately apparent. The overall smoothness of the light distribution indicates a relatively evolved system, possibly with a diminished rate of on-going star formation. There is a pronounced cigar shape to the galaxy. There does not appear to be any ongoing merger events or major disturbances to its structure.
