This galaxy appears to be a relatively smooth and rounded system. The central region exhibits a concentrated, bright core, suggesting a possible bulge component. The overall color profile trends towards redder hues in the central regions, with bluer colors becoming faintly visible at the edges. Faint disturbances are seen along the edge of the galaxy. The morphology indicates a possible recent or ongoing interaction or minor merger event. This would contribute to active star formation, but may not be visually apparent due to dust obscuration.
