The galaxy presents as a roughly elliptical structure with a bright, concentrated central bulge. There is a noticeable color gradient from the core outwards. The core appears to be a yellow/orange hue, suggesting an older stellar population. Moving outwards, the color shifts towards a bluer tint, possibly indicating regions of more recent star formation. While the overall structure is smooth, there are hints of a disk-like component or faint spiral arms in the outer regions, though these features are not sharply defined. The galaxy exhibits a degree of disturbance, perhaps due to a minor galactic interaction. There is no strong evidence of a major ongoing merger.
