The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its overall color is yellowish-white, suggesting an older stellar population with fewer young, massive stars. The isophotes appear largely regular and elliptical, indicating a well-mixed stellar distribution. There's a subtle color gradient, with the core exhibiting a slightly more golden hue. Faint extensions are observed from the central region of the galaxy, indicating low luminosity outer regions. No distinct spiral arm structure or prominent dust lanes are visible. There is no obvious active galactic nucleus based on the even illumination. Overall, the galaxy presents as a passively evolving system, with a significant fraction of its stars likely being old and metal-rich. There is no significant evidence of recent or ongoing major mergers.
