The galaxy presents a generally smooth morphology, with a concentrated central bulge exhibiting a yellow-orange hue. This coloration likely indicates an older stellar population dominating the bulge region. The galaxy is relatively symmetric and compact, appearing more elliptical than spiral. There's a subtle color gradient, transitioning from the yellower core to a slightly bluer periphery, which hints at the presence of some younger, star-forming regions in the outer disk. The galaxy does not show any signs of major ongoing mergers or significant tidal disturbances.
