The galaxy presents as an elliptical type, exhibiting a largely smooth, centralized luminosity distribution. The overall shape appears somewhat rounded, but shows a subtle elongation or deviation from perfect circularity. A dominant, yellowish core is visible, suggesting a high concentration of older stellar populations. The outer regions fade gradually, transitioning to a fainter halo or envelope. There is little evidence of distinct spiral arms, prominent dust lanes, or significant star-forming regions within the galaxy's structure. The overall morphology suggests a relatively quiescent galaxy with minimal ongoing star formation activity. There is a slight hint of disturbance, such as a tidal tail, however it is a low probability.
