The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a generally round morphology. There is a concentration of light toward the center, indicating a bright galactic nucleus. The galaxy displays a yellow-red hue, suggesting an older stellar population, potentially with lower levels of ongoing star formation, as well as an abundance of heavier elements within the galaxy. There is no immediately apparent spiral structure or significant dust lanes visible. Faint irregularities hint at a potential interaction, but there is no clear evidence for a major merger event currently occurring. The gradual decrease in luminosity from the core to the outer edges indicates a smooth stellar density gradient.
