The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular type. It exhibits an elongated shape, appearing cigar-like, with a gradual increase in luminosity towards the central region. The core displays a concentrated, bright, yellowish-white hue. Moving outward from the core, the light gradually fades and reddens, suggesting an aging stellar population. There is no evidence of prominent spiral arms or significant dust lanes. No tidal tails or distortions are apparent, indicating minimal recent or ongoing mergers. The overall structure suggests a relatively evolved galaxy with little current star formation.
